stele – -Translation – Keybot Dictionary

  Disk Detective | Joacă-...  

Show textShow cached sourceOpen source URL	Sistemul Solar, stele, sateliţi, astronomie
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The Solar System, stars, satellites, the science of astronomy
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The Solar System, stars, satellites, the science of astronomy

  Disk Detective | Joacă-...  

Show textShow cached sourceOpen source URL	Disk Detective observă stelele în încercarea de a descoperi discuri de materie şi praf cosmic, asemănătoare câmpului nostru de asteroizi. Aceste discuri indică faptul că stelele aferente se află într-un stadiu incipient de formare a unui sistem planetar.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	In Disk Detective, you look at stars to find dusty debris disks, which are similar to our asteroid field. These disks suggest that the related stars are in the early stages of forming planetary systems. Learning more about these stars can tell us how our Solar System was formed.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	In Disk Detective, you look at stars to find dusty debris disks, which are similar to our asteroid field. These disks suggest that the related stars are in the early stages of forming planetary systems. Learning more about these stars can tell us how our Solar System was formed.

  Space Awareness  

Show textShow cached sourceOpen source URL	Descoperă profesii spaţiale Visezi să ajungi printre stele? Află cum poţi contribui la studiul şi explorarea spaţiului.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ontdek RuimteCarrières Richten op de sterren? Zie hoe jij kunt bijdragen aan ruimtewetenschap en -verkenning.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Poznaj kosmiczne kariery Mierzysz w gwiazdy? Zobacz, jak można wnieść wkład do nauk o kosmosie i jego eksploracji.

  Razele X dezvăluie găur...  

Show textShow cached sourceOpen source URL	Razele X dezvăluie găuri negre dansând cu stele normale
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	X-rays Uncover Black Holes Dancing With Normal Stars
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Röntgenstrahlen enthüllen Tanz Schwarzer Löcher mit normalen Sternen
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Los rayos X descubren agujeros negros bailando con estrellas normales
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Röntgenfoto van dans tussen zwart gat en ster
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	X-rays Uncover Black Holes Dancing With Normal Stars
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	X-rays Uncover Black Holes Dancing With Normal Stars

  Urme ale unei planete a...  

Show textShow cached sourceOpen source URL	În 2014, oamenii de știință au descoperit două breșe în discul unei stele tinere. Liniile punctate din imaginea de mai sus arată cele două breșe.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	En 2014, des scientifiques ont découvert deux grands espaces vides dans le disque entourant une jeune étoile. Les lignes pointillées sur l’image indiquent où se situent les deux brèches.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Im Jahr 2014 entdeckten die Wissenschaftler zwei große Lücken in der Scheibe eines jungen Sterns. Die gestrichelten Linien auf dem obigen Bild markieren, wo sich die beiden Lücken befinden.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	En 2014, unos científicos descubrieron dos grandes huecos en el disco alrededor de una estrella joven. Las líneas punteadas de la imagen marcan la ubicación de los dos huecos.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Em 2014, os cientistas descobriram dois grandes intervalos no disco à volta de uma estrela jovem. As linhas a tracejado marcam a sua localização.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	In 2014 ontdekten wetenschappers twee grote lege plekken in de schijf rond een jonge ster. De gestreepte lijnen in de afbeelding hierboven geven aan waar de twee lege plekken zijn.

  Disk Detective | Joacă-...  

Show textShow cached sourceOpen source URL	Planetele sunt formate din nori imenşi de gaze, praf şi fragmente de rocă, nori care capătă forma unor discuri ce se rotesc în jurul stelelor din centru. Pentru a afla unde se formează planete sau unde acestea există deja, trebuie să căutăm stele înconjurate de astfel de discuri.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Planets are formed from vast clouds of gas, dust, and chunks of rock clouds that take the shape of disks with stars in the centre. It is possible to tell where planets are forming and where planets probably exist by searching for specific stars surrounded by these types of disks. Computers often confuse debris disks around stars with other astronomical objects. Your help is needed to find the stars that actually have these disks around them in galaxies or nebulae.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Planets are formed from vast clouds of gas, dust, and chunks of rock clouds that take the shape of disks with stars in the centre. It is possible to tell where planets are forming and where planets probably exist by searching for specific stars surrounded by these types of disks. Computers often confuse debris disks around stars with other astronomical objects. Your help is needed to find the stars that actually have these disks around them in galaxies or nebulae.

  Astronomii au elucidat ...  

Show textShow cached sourceOpen source URL	Cele mai atrăgătoare stele din univers
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Une cacahuète au centre de notre Galaxie ?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Romance estelar destinado a acabar en desastre
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Cosmic Tidal Wave Wakes Up Sleeping Galaxies

  Urme ale unei planete a...  

Show textShow cached sourceOpen source URL	Urme ale unei planete abia formate au fost observate în jurul unei stele tinere
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Des empreintes de bébé-planètes décelées autour d’une jeune étoile
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Fußabdrücke von Babyplaneten in der Nähe eines jungen Sterns gesichtet
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Huellas de planetas bebé alrededor de una estrella joven
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Pegadas de planetas bebés à volta de uma estrela jovem
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Voetafdrukken van Babyplaneten Gevonden om een Jonge Ster

  Razele X dezvăluie găur...  

Show textShow cached sourceOpen source URL	După ce au studiat multe stele din Calea Lactee, astronomii au descoperit că stelele cu cat sunt mai mari cu atăt au mai multe șanse să aibe în companie o altă stea.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	After studying many stars within the Milky Way, astronomers have found evidence that the more massive a star is, the more likely it is to have a companion.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Nachdem nun so viele Sterne unserer Milchstraße untersucht wurden, haben die Astronomen Hinweise dafür gefunden, dass je massiver ein Stern ist, desto wahrscheinlicher ist es, dass er einen Begleiter hat.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Después de estudiar muchas estrellas en la Vía Láctea, los astrónomos han encontrado indicios de que cuanto más masiva es una estrella, mayor es la probabilidad de que tenga una compañera.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Na het bestuderen van vele sterren in de Melkweg hebben astronomen bewijs gevonden dat hoe zwaarder een ster is, des te waarschijnlijker het is dat hij gezelschap heeft van een andere ster.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	After studying many stars within the Milky Way, astronomers have found evidence that the more massive a star is, the more likely it is to have a companion.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	After studying many stars within the Milky Way, astronomers have found evidence that the more massive a star is, the more likely it is to have a companion.

  Imaginile din copilăria...  

Show textShow cached sourceOpen source URL	Astronomii au capturat o nouă fotografie care ilustrează nașterea a noi planete în jurul unei stele tinere îndepârtate!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Talk about your ultimate baby picture. Astronomers have snapped a new photograph showing new planets being born around a distant young star!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Des astronomes ont pris une nouvelle photo montrant des planètes en train de se former autour d’une jeune étoile !
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Wie sieht dein ultimatives Babybild aus? Astronomen haben einen Schnappschuss von neuen, gerade geborenen Planeten um einen jungen Stern gemacht!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ya puedes decir lo que quieras sobre tu mejor fotografía de bebés. ¡Los astrónomos han tomado una nueva imagen que muestra planetas que están naciendo alrededor de una lejana estrella joven!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Os astrónomos obtiveram recentemente, esta nova fotografia mostrando o nascimento de novos planetas em torno de uma estrela jovem.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Over je ultieme babyfoto gesproken… Sterrenkundigen hebben een nieuw kiekje gemaakt van nieuwe planeten die rond een verre, jonge ster worden geboren!

  Oul unui dinozaur cosmi...  

Show textShow cached sourceOpen source URL	Firecracker pare suficient de mare pentru a da naștere în viitor unui nou roi globular. Conține suficient material pentru a da naștere la 50 de milioane de stele asemănătoare soarelui nostru. Până acum nu s-a format nici o stea în acest nor.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Le Pétard semble assez gros pour former un nouvel amas globulaire dans le futur. Il contient assez de matière pour former 50 millions d’étoiles comme notre Soleil ! Mais pour l’instant aucune nouvelle étoile ne s’est formée dans le nuage. C’est comme un « œuf cosmique » sur le point d’éclore.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	El Petardo parece ser suficientemente grande como para crear un nuevo cúmulo globular entero en el futuro. ¡Contiene suficiente material para crear cincuenta millones de estrellas como nuestro Sol! Pero todavía no han nacido nuevas estrellas en la nube. Es como un “huevo cósmico”, a punto de abrirse.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	O “Petardo” parece ser suficientemente grande para criar no futuro um novo enxame globular. Contém material suficiente para criar cinquenta novas estrelas como o nosso Sol! No entanto ainda não nasceram novas estrelas nesta nuvem. É como um “ovo cósmico”, pronto a eclodir.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	De Vuurpijl lijkt groot genoeg om in de toekomst een heel nieuw bolvormige sterrenhoop te maken. Het bevat genoeg materiaal om vijftig miljoen sterren zoals onze Zon te maken! Maar er zijn nog geen nieuwe sterren geboren in deze wolk. Het is net een ‘kosmisch ei’, klaar om uit te komen.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The Firecracker appears to be big enough to create an entire new globular cluster in the future. It contains enough material to make fifty million stars like our Sun! But no new stars have yet been born in the cloud. It’s like a ‘cosmic egg’, ready to hatch.

  Razele X dezvăluie găur...  

Show textShow cached sourceOpen source URL	Fiecare sistem binar cu raze X este compus dintr-o stea normală și o stea ce a trecut de capătul vieții sale. Aceste companioane sunt de cele mai multe ori de tip stele neutrine dar se întămplă să fie și găuri negre.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Each X-ray binary is made up of a normal star and a star which has passed beyond the end of its life. These companions are exotic things, most commonly a neutron star but sometimes, a black hole.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Jedes Röntgendoppelsternpaar besteht aus einem normalen Stern und einem Stern, dessen Leben bereits vorbei ist. Diese Begleiter sind exotische Objekte, meistens ein Neutronenstern aber manchmal auch ein Schwarzes Loch.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Cada binaria de rayos X está constituida por una estrella normal y una estrella que ha superado el final de su vida. Estas compañeras son cosas exóticas, siendo habitualmente una estrella de neutrones, aunque a veces se trata de un agujero negro.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Elke röntgendubbelster bestaat uit een normale ster en een ster die al voorbij het einde van zijn leven is. Dat betekent dat hij een exotisch object is geworden; meestal een neutronenster, en soms een zwart gat.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Each X-ray binary is made up of a normal star and a star which has passed beyond the end of its life. These companions are exotic things, most commonly a neutron star but sometimes, a black hole.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Each X-ray binary is made up of a normal star and a star which has passed beyond the end of its life. These companions are exotic things, most commonly a neutron star but sometimes, a black hole.

  Cărămizile care stau la...  

Show textShow cached sourceOpen source URL	Bine, moleculele organice sunt foarte fragile. Ele nu supraviețuesc în general condițiilor dificile din preajma stelelor noi formate. Cu toate acestea, oamenii de știință au descoperit o cantitate mare de molecule organice în jurul unei stele tinere și îndepărtate.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	C’est parce que les molécules organiques sont très fragiles. Elles survivent rarement aux conditions extrêmes entourant les nouvelles étoiles. Cependant, les scientifiques viennent de détecter des quantités énormes de molécules organiques autour d’une « jeune » étoile lointaine.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Bueno, las moléculas orgánicas son muy frágiles. A menudo no sobreviven a las duras condiciones que rodean a las estrellas recién nacidas. Sin embargo, los científicos acaban de detectar enormes cantidades de moléculas orgánicas alrededor de una joven y lejana estrella.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Na realidade, as moléculas orgânicas são extremamente frágeis. Não sobrevivem facilmente às duras condições que rodeiam as estrelas recém-nascidas. Apesar disso, os cientistas acabaram de detectar grandes quantidades de moléculas orgânicas em torno de uma jovem estrela distante.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Nou, organische moleculen zijn heel breekbaar. Vaak overleven ze de barre omstandigheden in de buurt van nieuwe sterren niet. Echter, wetenschappers hebben net grote hoeveelheden organische moleculen ontdekt in de buurt van een jonge en ver weg staande ster.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ами, органичните молекули са много деликатни. Често те не могат да оцелеят в неблагоприятните условия около новородените звезди. Въпреки това, учените тъкмо са открили огромни количества органични молекули около една млада и далечна звезда.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Well, organic molecules are very fragile. They don’t often survive the harsh conditions surrounding new-born stars. However, scientists have just detected huge amounts of organic molecules around a young and distant star.

  O schimbare majoră | Ci...  

Show textShow cached sourceOpen source URL	Roiurile conțin zeci de mii de stele vechi formate cam în aceeași perioadă și cam din același tip de material. Însă, uneori, ele conțin stele ce par surprinzător de tinere, ceea ce ne face să ne întrebăm dacă aceste roiuri de stele sunt cu adevărat relicve ale trecutului așa cum credeam.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Globular clusters contain tens of thousands of ancient stars that all formed around the same time, from the same material. But strangely, these clusters sometimes contain stars that look suspiciously young, raising the question: are these clusters really the ancient relics that we believe?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Kugelsternhaufen enthalten zehntausende von alten Sternen, die alle etwa zur gleichen Zeit und aus dem gleichen Material gebildet wurden. Aber seltsamerweise enthalten diese Haufen manchmal Sterne, die überraschend jung aussehen und die Frage aufwerfen: Sind diese Haufen tatsächlich so alt wie wir denken?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Los cúmulos globulares contienen decenas de miles de estrellas antiguas, todas ellas formadas alrededor de la misma época, a partir del mismo material. Pero, extrañamente, estos cúmulos a veces contienen estrellas que parecen sospechosamente jóvenes, provocando la pregunta: ¿son estos cúmulos realmente las reliquias antiguas que creemos que son?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Gli ammassi globulari contengono decine di migliaia di vecchie stelle, che si sono formate tutte circa nello stesso periodo dallo stesso materiale. Eppure, stranamente, ogni tanto questi ammassi contengono stelle che sembrano piuttosto giovani, cosicché la domanda sorge spontanea: davvero questi ammassi sono quei fossili antichi che crediamo noi?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Enxames globulares contêm dezenas de milhares de estrelas antigas que se formaram na mesma época, do mesmo material. Mas curiosamente, esses enxames contêm por vezes estrelas estranhamente jovens, levantando a questão: são na realidade esses enxames as antigas relíquias que pensamos serem?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Bolvormige sterrenhopen (of bolhopen) bevatten tienduizenden oude sterren die allemaal rond hetzelfde tijdstip zijn gevormd, vanuit hetzelfde materiaal. Maar gek genoeg bevatten deze bolhopen soms ook sterren die er verbazingwekkend jong uit zien. Zijn die bolhopen dus echt wel zo oud?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Globular clusters contain tens of thousands of ancient stars that all formed around the same time, from the same material. But strangely, these clusters sometimes contain stars that look suspiciously young, raising the question: are these clusters really the ancient relics that we believe?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Gromady kuliste zawierają dziesiątki tysięcy bardzo wiekowych gwiazd, które powstały w tym samym okresie i z tej samej materii. Jednak czasem odnajdujemy w takich gromadach gwiazdy stosunkowo młode, zupełnie niepasujące do reszty. Powoduje to powstanie pytania czy gromady otwarte są naprawdę takimi starymi tworami, za jakie je uważamy.

  Frumusețe în roz | Cite...  

Show textShow cached sourceOpen source URL	Fotografia de mai sus ilustrează un nor de praf și gaz, numit de astronomi „maternitate stelară”. În adâncul acestui nor roz se nasc noi stele; din nefericire, lumina vizibilă a acestor stele nou formate nu poate fi înregistrată de VLT, aceasta fiind blocată de un strat gros de praf.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Obviously, what we're looking at isn't really a party in space, although that sounds like a lot of fun! What this picture actually shows is a spectacular cloud of gas and dust that astronomers call a stellar nursery. That´s because deep inside this pretty pink cloud, new stars are flaring into life. Unfortunately the thick dust traps and visible light from these newborn stars, so the Very Large Telescope can't see them.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Obviamente, lo que estamos viendo no es realmente una fiesta en el espacio, ¡aunque eso sería muy divertido! Lo que la imagen nos muestra de verdad es una espectacular nube de gas y polvo que los astrónomos llaman vivero estelar. Esto es así porque a gran profundidad en el interior de esta bonita nube rosa, hay nuevas estrellas naciendo a la vida. Por desgracia, el polvo grueso atrapa la luz visible de estas estrellas recién nacidas, así que el Very Large Telescope no las puede ver.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ovviamente quella che stai guardando non è una festa spaziale! In realtà questa fotografia ci mostra una spettacolare nube di gas e polvere, quello che gli astronomi chiamano un "asilo nido" stellare. Infatti, nelle profondità di questa splendida nube rosa vengono al mondo tante nuove stelle. Purtroppo, gli strati spessi di polvere bloccano la luce visibile di queste nuove stelle, e con il Very Large Telescope non possiamo vederle.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Embora isto nos pareça muito divertido, obviamente que não estamos a olhar para uma festa no espaço! O que na realidade esta imagem mostra é uma espetacular nuvem de gás e poeira, a que os astrónomos chamam de maternidade estelar. Isto deve-se a que a grande profundidade, no interior desta belíssima nuvem rosa estarem a nascer novas estrelas. Infelizmente, estas estrelas recém-nascidas não conseguem ser vistas pelo Very Large Telescope devido à espessa camada de poeira que oculta a sua luz.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Natuurlijk is dit niet echt een feestje in de ruimte, hoewel dat best leuk zou kunnen zijn! Wat de foto laat zien is een spectaculaire wolk van gas en stof die sterrenkundigen een 'stellaire kraamkamer' noemen. Diep in deze mooie roze wolk worden nieuwe sterren geboren. Helaas houdt het dikke stof het licht van sommige van deze nieuwgeboren sterren tegen, waardoor de Very Large Telescope hen niet kan zien.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Obviously, what we're looking at isn't really a party in space, although that sounds like a lot of fun! What this picture actually shows is a spectacular cloud of gas and dust that astronomers call a stellar nursery. That´s because deep inside this pretty pink cloud, new stars are flaring into life. Unfortunately the thick dust traps and visible light from these newborn stars, so the Very Large Telescope can't see them.

  Vânătorii de supernove ...  

Show textShow cached sourceOpen source URL	Explozia unei stele masive poartă numele de supernovă. Ele sunt printre cele mai violente evenimente din Univers și sunt atât de strălucitoare încât pentru scurt timp pot întrece în luminozitate galaxii intregi după care se estompează pe parcursul câtorva săptămâni sau chiar luni.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The explosion of a massive star is called a supernova. They are amongst the most energetic events in the Universe and are so bright that they often briefly outshine an entire galaxy before fading from view over several weeks or months. During this short period, a supernova can give off as much energy as the Sun will in its entire lifetime!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Die Explosion eines massereichen Sterns nennt man eine Supernova. Supernovae gehören zu den energiereichsten Ereignissen im Universum und sind so hell, dass sie oft für eine kurze Zeit eine ganze Galaxie überstrahlen bevor sie dann über einen Zeitraum von mehreren Wochen oder Monaten hin aus dem Blickfeld verschwinden. Während dieser kurzen Zeit kann eine Supernova so viel Energie abgeben wie die Sonne während ihrer gesamten Lebenszeit!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	La explosión de una estrella masiva se llama supernova. Son de los sucesos más energéticos del Universo y son tan brillantes que a menudo brillan brevemente mucho más que una galaxia entera, antes de ir perdiendo brillo a lo largo de varias semanas o meses. ¡Durante este corto periodo de tiempo, una supernova puede proporcionar tanta energía como la que dará el Sol a lo largo de su vida entera!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	A explosão de uma estrela de grande massa é chamada uma supernova. Este é um dos eventos mais energéticos do universo e é tão brilhante que muitas vezes ofusca uma galáxia inteira, antes de desaparecer de vista ao longo de várias semanas ou meses. Durante este curto período, uma supernova pode libertar tanta energia como o Sol durante toda a sua vida!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	De ontploffing van een zware ster heet een supernova. Het zijn de meest gewelddadige gebeurtenissen in het heelal. Supernova-explosies zijn zo helder, dat ze vaak een heel sterrenstelsel oplichten. Na een paar weken of maanden neemt de helderheid weer af. Tijdens die korte periode straalt de supernova evenveel energie uit als de zon in zijn hele leven!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The explosion of a massive star is called a supernova. They are amongst the most energetic events in the Universe and are so bright that they often briefly outshine an entire galaxy before fading from view over several weeks or months. During this short period, a supernova can give off as much energy as the Sun will in its entire lifetime!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Zjawisko eksplozji masywnej gwiazdy nazywamy supernową. Takie kosmiczne wybuchy produkują ogromne ilości energii, a światło, które im towarzyszy może oświetlić całą galaktykę na czas kilku tygodni lub miesięcy. Tylko w trakcie tego czasu supernowa może emitować tak tyle energii, ile Słońce daje przez okres całego swego życia!

  O schimbare majoră | Ci...  

Show textShow cached sourceOpen source URL	Stelele din centrul acestei fotografii sunt incredibil de vechi. Ele ardeau cu mult înainte ca primul om să calce pe Pământ, chiar cu mult înainte ca Pământul să existe. Această grupare de stele, numită roi globular, are o vechime de 10 miliarde de ani, ea fiind aproape la fel de veche ca Universul.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The ball of stars at the centre of this photograph is unbelievably old. These stars were burning before the first humans walked on Earth, before there even was an Earth. This group of stars, called a globular cluster, is actually 10 billion years old — that's almost as old as the universe itself!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Der Sternenball in der Mitte dieses Fotos ist unglaublich alt. Diese Sterne leuchteten schon bevor der erste Mensch auf der Erde umherlief, ja noch bevor es überhaupt eine Erde gab. Diese Sternengruppe, die als Kugelsternhaufen bezeichnet wird, ist tatsächlich 10 Milliarden Jahre alt – das ist fast so alt wie das Weltall selbst!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	La bola de estrellas del centro de esta fotografía es increíblemente vieja. Estas estrellas estaban encendidas antes de que los primeros humanos caminaran sobre la Tierra, incluso antes de que hubiera Tierra. Este grupo de estrellas, llamado cúmulo globular, tiene realmente 10 mil millones de años de edad - ¡eso es casi tan viejo como el propio universo!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	La palla di stelle al centro di questa fotografia è incredibilmente vecchia. Prima che i primi esseri umani si aggirassero sulla Terra, queste stelle stavano già bruciando. Un gruppo di stelle come questo si chiama ammasso globulare, e ha circa 10 miliardi di anni - in pratica quasi l'età dell'Universo!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	A bola de estrelas no centro desta fotografia é incrivelmente antiga. Estas estrelas ardiam antes dos primeiros seres humanos andarem na Terra, mesmo antes de haver uma Terra. Esse grupo de estrelas, chamado de enxame globular, tem na realidade 10 milhares de milhões de anos — quase tão antigo como o próprio universo!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	De hoop sterren in het midden van de foto is ongelofelijk oud. Deze sterren brandden al voordat de eerste mensen op aarde waren, zelfs voordat er een aarde was. Deze groep sterren noemen we een bolvormige sterrenhoop. Hij is 10 miljard jaar oud, bijna zo oud als het heelal zelf!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The ball of stars at the centre of this photograph is unbelievably old. These stars were burning before the first humans walked on Earth, before there even was an Earth. This group of stars, called a globular cluster, is actually 10 billion years old — that's almost as old as the universe itself!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Zbiorowisko gwiazd prezentowane pośrodku powyższego zdjęcia jest niewyobrażalnie stare. Gwiazdy te powstały bowiem na długo przed tym, gdy człowiek zaczął chodzić po Ziemi, czy nawet przed jej powstaniem. Przedstawione zgrupowanie gwiazd nazywane jest przez astronomów gromadą kulistą i ma 10 miliardów lat, czyli niemal tyle, ile liczy sobie wiek Wszechświata!

  O fotografie de familie...  

Show textShow cached sourceOpen source URL	Raportat la stele, oamenii există doar de foarte, foarte puțin timp. Stelele trăiesc mii, milioane și chiar miliarde de ani. Prin urmare, este imposibil să urmărim nașterea, viața și moartea aceleași stele, dar putem observa stele diferite aflate în etape diferite ale vieții lor.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Compared to stars, humans have only been around for the blink of an eye. Stars live for thousands, millions or even billions of years. So, we can’t possibly witness the birth, life and death of the same star. However, we can observe stars at different stages of life.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Comparée aux étoiles, l’histoire de l’humanité ne dure pas plus longtemps qu’un clignement d’œil. Par contre, certaines étoiles « vivent » pendant des milliers d’années, d’autres pendant plus de 10 milliards d’années. Nous ne pouvons donc pas être les témoins de la formation d’une étoile jusqu’à ce qu’elle disparaisse. Mais nous pouvons observer les étoiles à différents stades de leur évolution.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Im Vergleich zu Sternen gibt es Menschen erst seit einem Zeitraum eines Wimpernschlags. Sterne leben Tausende, Millionen oder gar Milliarden von Jahren. Daher können wir keinesfalls die Geburt, das Leben und den Tod eines einzelnen Sterns erleben. Allerdings können wir Sterne zu verschiedenen Stadien ihres Lebens beobachten.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Comparados con estrellas, los humanos han existido sólo durante un abrir y cerrar de ojos. Las estrellas viven miles, millones o incluso miles de millones de años. Así que no es posible que podamos ser testigos del nacimiento, vida y muerte de la misma estrella. Sin embargo, podemos observar estrellas en diferentes momentos de la vida.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Rispetto alle stelle, infatti, gli esseri umani hanno una vita lunga appena un battito di ciglia. Le stelle vivono per migliaia, milioni o addirittura miliardi di anni. Di una specifica stella, non possiamo osservare nascita, vita e scomparsa: e tuttavia, possiamo osservare tante stelle diverse, ciascuna in uno stadio differente della propria esistenza.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Em comparação com as estrelas, os seres humanos existem apenas durante um piscar de olhos. As estrelas vivem milhares, milhões ou mesmo milhares de milhões de anos. Portanto, não nos é possível testemunhar o nascimento, a vida e a morte de uma determinada estrela. Podemos contudo observar estrelas em diversos pontos do seu ciclo de vida.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Vergeleken met sterren, bestaat de mensheid korter dan een flits. Sterren leven duizenden, miljoenen of zelfs miljarden jaren lang. Daarom kunnen we onmogelijk zien hoe een enkele ster geboren wordt, leeft en sterft. Maar we kunnen wel sterren bekijken op verschillende momenten van het leven van een ster.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ve srovnání s délkou života hvězd jsou lidé na světě jen mžik, tedy opravdu krátce. Hvězdný život je dlouhý, žijí tisíce, milióny nebo dokonce miliardy let. A my tedy nemůžeme být svědky zrození, života a smrti jedné a té samé hvězdy. Můžeme ale, stejně jako naši mimozemšťané, pozorovat více hvězd v různých fázích jejich života.

  Frumusețe în roz | Cite...  

Show textShow cached sourceOpen source URL	Fotografia de mai sus ilustrează un nor de praf și gaz, numit de astronomi „maternitate stelară”. În adâncul acestui nor roz se nasc noi stele; din nefericire, lumina vizibilă a acestor stele nou formate nu poate fi înregistrată de VLT, aceasta fiind blocată de un strat gros de praf.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Obviously, what we're looking at isn't really a party in space, although that sounds like a lot of fun! What this picture actually shows is a spectacular cloud of gas and dust that astronomers call a stellar nursery. That´s because deep inside this pretty pink cloud, new stars are flaring into life. Unfortunately the thick dust traps and visible light from these newborn stars, so the Very Large Telescope can't see them.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Obviamente, lo que estamos viendo no es realmente una fiesta en el espacio, ¡aunque eso sería muy divertido! Lo que la imagen nos muestra de verdad es una espectacular nube de gas y polvo que los astrónomos llaman vivero estelar. Esto es así porque a gran profundidad en el interior de esta bonita nube rosa, hay nuevas estrellas naciendo a la vida. Por desgracia, el polvo grueso atrapa la luz visible de estas estrellas recién nacidas, así que el Very Large Telescope no las puede ver.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ovviamente quella che stai guardando non è una festa spaziale! In realtà questa fotografia ci mostra una spettacolare nube di gas e polvere, quello che gli astronomi chiamano un "asilo nido" stellare. Infatti, nelle profondità di questa splendida nube rosa vengono al mondo tante nuove stelle. Purtroppo, gli strati spessi di polvere bloccano la luce visibile di queste nuove stelle, e con il Very Large Telescope non possiamo vederle.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Embora isto nos pareça muito divertido, obviamente que não estamos a olhar para uma festa no espaço! O que na realidade esta imagem mostra é uma espetacular nuvem de gás e poeira, a que os astrónomos chamam de maternidade estelar. Isto deve-se a que a grande profundidade, no interior desta belíssima nuvem rosa estarem a nascer novas estrelas. Infelizmente, estas estrelas recém-nascidas não conseguem ser vistas pelo Very Large Telescope devido à espessa camada de poeira que oculta a sua luz.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Natuurlijk is dit niet echt een feestje in de ruimte, hoewel dat best leuk zou kunnen zijn! Wat de foto laat zien is een spectaculaire wolk van gas en stof die sterrenkundigen een 'stellaire kraamkamer' noemen. Diep in deze mooie roze wolk worden nieuwe sterren geboren. Helaas houdt het dikke stof het licht van sommige van deze nieuwgeboren sterren tegen, waardoor de Very Large Telescope hen niet kan zien.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Obviously, what we're looking at isn't really a party in space, although that sounds like a lot of fun! What this picture actually shows is a spectacular cloud of gas and dust that astronomers call a stellar nursery. That´s because deep inside this pretty pink cloud, new stars are flaring into life. Unfortunately the thick dust traps and visible light from these newborn stars, so the Very Large Telescope can't see them.

  O fotografie de familie...  

Show textShow cached sourceOpen source URL	Punctul luminos din centrul acestei imagini este Cygnus X-3. Acesta este format din două obiecte care se învârt unul în jurul celuilalt; unul este o stea de vârstă medie, iar cel de-al doilea reprezintă rămașițele unei stele masive, care a murit.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	The bright point of light at the centre of the picture is Cygnus X-3 (“sig-nus”). It includes two objects circling each other; one is a middle aged star, the other is what remains of a massive star that died. We call this type of object an 'X-ray binary system', because it shines brightly in X-ray light.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Le plus grand point brillant au milieu de l’image est Cygnus X-3 (« sig-nus »). Cygnus X-3 est formé de deux astres tournant l’un autour de l’autre : l’un est une étoile d’âge moyen et l’autre est ce qu’il reste d’une étoile massive qui a explosé. L’ensemble s’appelle un « système binaire en rayons X » parce qu’il émet beaucoup d’énergie aux fréquences X de la lumière.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Der helle Punkt in der Bildmitte ist Cygnus X-3. Er beinhaltet zwei Objekte, die sich gegenseitig umkreisen. Eins davon ist ein Stern im besten Alter, das andere ist der Rest eines massereichen Sterns nach seinem Tod. Man nennt so ein Objekt einen "Röntgen-Doppelsternsystem", weil es besonders hell im Röntgenlicht leuchtet.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	El punto brillante de luz del centro de la imagen es Cygnus X-3. Incluye dos objetos que giran uno alrededor del otro: uno es una estrella de edad media, el otro son los restos de una estrella masiva que murió. Llamamos a este tipo de objeto un “sistema binario de rayos X” porque brilla intensamente en luz de rayos X.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Il punto brillante al centro dell’immagine è Cygnus X-3. In realtà, è costituito da due sorgenti che ruotano una intorno all’altra: una è una stella di mezz’età, mentre l’altra è quel che resta di una stella molto massiva, ormai spenta. Un sistema di questo genere è chiamato “sistema binario a raggi X”, perché appare splendere, appunto, quando viene osservato nei raggi X.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	O ponto de luz brilhante ao centro da imagem é Cisne X-3. Inclui dois objetos que se orbitam mutuamente; um é uma estrela de meia-idade, o outro é o que resta de uma estrela maciça que já morreu. Chamamos a este tipo de objeto um “sistema binário de raios X”, porque ele brilha fortemente na frequência dos raios X.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Het felle lichtpunt in het midden van de foto is Cygnus X-3 (zeg: sig-nus). Ook zie je twee andere objecten, die om elkaar draaien; de ene is een ster van gemiddelde leeftijd, de ander is wat overblijft van een heel zware, dode ster. We noemen een groep als deze een ‘röntgendubbelster’, omdat het zo fel schijnt in röntgenstraling.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ten jasný světelný bod ve středu fotografie je Cygnus X-3 („sig-nus"). Obsahuje dva objekty, které se otáčí jeden kolem druhého, jeden je středně stará hvězda a ten druhý - to jsou zbytky po výbuchu obrovské hvězdy, která zemřela. Takový objekt nazýváme „rentgenový binární systém", protože jasně září v rentgenové části světelného spektra.

  Razele X dezvăluie găur...  

Show textShow cached sourceOpen source URL	Majoritatea stelelor din Calea Lactee nu sunt solitare, precum este Soarele nostru. 8 din 10 stele masive au una sau mai multe stele ca și companioane. O pereche de stele care orbitează una în jurul celeilalte poartă numele de sistem binar.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Die meisten Sterne unserer Milchstraße schweben nicht wie unsere Sonne allein durch das Weltall. Ein riesiger Anteil der massivsten Sterne, nämlich acht von zehn, haben einen oder mehrere Begleitsterne. Umkreist sich ein Sternenpaar, so nennen wir das ein Doppelsternsystem. Dieses Foto zeigt die auffällige Spiralgalaxie M51. Jeder der so lebendig leuchtenden lilafarbenen Lichtpunkte, die wir auf diesem Bild glitzern sehen, steht für einen besonderen Doppelsternsystemtyp. Wir nennen sie Röntgendoppelsterne, da es sich um Sternenpaare handelt, die Röntgenlicht aussenden.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	La mayoría de las estrellas de la galaxia la Vía Láctea no son como nuestro Sol, que flota solo por el espacio. Hasta 8 de cada 10 de las estrellas más masivas tienen una o más estrellas compañeras. Una pareja de estrellas en órbita una alrededor de la otra recibe el nombre de “sistema binario”. Esta fotografía muestra la majestuosa galaxia espiral llamada Messier 51. Cada punto de vívida luz púrpura que vemos resplandeciendo en esta imagen representa un tipo especial de sistema binario. Les llamamos “binarias de rayos X” porque son parejas de estrellas que resplandecen en luz de rayos X.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	De meeste sterren in de Melkweg zweven niet zoals onze Zon in hun eentje door de ruimte. Acht op de tien zware sterren hebben gezelschap van één of meer sterren. Een paartje sterren dat om elkaar heen draait noemen we een dubbelster. Deze foto laat het flamboyante spiraalvormige sterrenstelsel Messier 51 zien. Elk puntje dat we in levendig paars zien schijnen in dit plaatje is een speciaal soort dubbelster. We noemen ze ‘röntgendubbelsterren’, omdat ze hun licht uitstralen in de vorm van röntgenstraling.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.

  Razele X dezvăluie găur...  

Show textShow cached sourceOpen source URL	Majoritatea stelelor din Calea Lactee nu sunt solitare, precum este Soarele nostru. 8 din 10 stele masive au una sau mai multe stele ca și companioane. O pereche de stele care orbitează una în jurul celeilalte poartă numele de sistem binar.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Die meisten Sterne unserer Milchstraße schweben nicht wie unsere Sonne allein durch das Weltall. Ein riesiger Anteil der massivsten Sterne, nämlich acht von zehn, haben einen oder mehrere Begleitsterne. Umkreist sich ein Sternenpaar, so nennen wir das ein Doppelsternsystem. Dieses Foto zeigt die auffällige Spiralgalaxie M51. Jeder der so lebendig leuchtenden lilafarbenen Lichtpunkte, die wir auf diesem Bild glitzern sehen, steht für einen besonderen Doppelsternsystemtyp. Wir nennen sie Röntgendoppelsterne, da es sich um Sternenpaare handelt, die Röntgenlicht aussenden.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	La mayoría de las estrellas de la galaxia la Vía Láctea no son como nuestro Sol, que flota solo por el espacio. Hasta 8 de cada 10 de las estrellas más masivas tienen una o más estrellas compañeras. Una pareja de estrellas en órbita una alrededor de la otra recibe el nombre de “sistema binario”. Esta fotografía muestra la majestuosa galaxia espiral llamada Messier 51. Cada punto de vívida luz púrpura que vemos resplandeciendo en esta imagen representa un tipo especial de sistema binario. Les llamamos “binarias de rayos X” porque son parejas de estrellas que resplandecen en luz de rayos X.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	De meeste sterren in de Melkweg zweven niet zoals onze Zon in hun eentje door de ruimte. Acht op de tien zware sterren hebben gezelschap van één of meer sterren. Een paartje sterren dat om elkaar heen draait noemen we een dubbelster. Deze foto laat het flamboyante spiraalvormige sterrenstelsel Messier 51 zien. Elk puntje dat we in levendig paars zien schijnen in dit plaatje is een speciaal soort dubbelster. We noemen ze ‘röntgendubbelsterren’, omdat ze hun licht uitstralen in de vorm van röntgenstraling.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.

  O schimbare majoră | Ci...  

Show textShow cached sourceOpen source URL	Roiurile conțin zeci de mii de stele vechi formate cam în aceeași perioadă și cam din același tip de material. Însă, uneori, ele conțin stele ce par surprinzător de tinere, ceea ce ne face să ne întrebăm dacă aceste roiuri de stele sunt cu adevărat relicve ale trecutului așa cum credeam.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Globular clusters contain tens of thousands of ancient stars that all formed around the same time, from the same material. But strangely, these clusters sometimes contain stars that look suspiciously young, raising the question: are these clusters really the ancient relics that we believe?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Kugelsternhaufen enthalten zehntausende von alten Sternen, die alle etwa zur gleichen Zeit und aus dem gleichen Material gebildet wurden. Aber seltsamerweise enthalten diese Haufen manchmal Sterne, die überraschend jung aussehen und die Frage aufwerfen: Sind diese Haufen tatsächlich so alt wie wir denken?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Los cúmulos globulares contienen decenas de miles de estrellas antiguas, todas ellas formadas alrededor de la misma época, a partir del mismo material. Pero, extrañamente, estos cúmulos a veces contienen estrellas que parecen sospechosamente jóvenes, provocando la pregunta: ¿son estos cúmulos realmente las reliquias antiguas que creemos que son?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Gli ammassi globulari contengono decine di migliaia di vecchie stelle, che si sono formate tutte circa nello stesso periodo dallo stesso materiale. Eppure, stranamente, ogni tanto questi ammassi contengono stelle che sembrano piuttosto giovani, cosicché la domanda sorge spontanea: davvero questi ammassi sono quei fossili antichi che crediamo noi?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Enxames globulares contêm dezenas de milhares de estrelas antigas que se formaram na mesma época, do mesmo material. Mas curiosamente, esses enxames contêm por vezes estrelas estranhamente jovens, levantando a questão: são na realidade esses enxames as antigas relíquias que pensamos serem?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Bolvormige sterrenhopen (of bolhopen) bevatten tienduizenden oude sterren die allemaal rond hetzelfde tijdstip zijn gevormd, vanuit hetzelfde materiaal. Maar gek genoeg bevatten deze bolhopen soms ook sterren die er verbazingwekkend jong uit zien. Zijn die bolhopen dus echt wel zo oud?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Globular clusters contain tens of thousands of ancient stars that all formed around the same time, from the same material. But strangely, these clusters sometimes contain stars that look suspiciously young, raising the question: are these clusters really the ancient relics that we believe?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Gromady kuliste zawierają dziesiątki tysięcy bardzo wiekowych gwiazd, które powstały w tym samym okresie i z tej samej materii. Jednak czasem odnajdujemy w takich gromadach gwiazdy stosunkowo młode, zupełnie niepasujące do reszty. Powoduje to powstanie pytania czy gromady otwarte są naprawdę takimi starymi tworami, za jakie je uważamy.

  Razele X dezvăluie găur...  

Show textShow cached sourceOpen source URL	Dacă cele două stele sunt suficient de apropiate atunci forța de gravitație a stelei exotice (steaua neutrino sau gaura neagră) poate atrage materia gazoasă a stelei normale, formând un inel în jurul său înainte de a fi inghițită de steaua masivă.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	If the stars are close enough together, the strong gravity of the exotic companion can drag gas off the normal star into a ring itself, before gobbling it up. When this happens the material is heated to over a million degrees and begins shining light as X-rays.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Sind beide Sterne nahe genug beieinander, kann die starke Anziehungskraft des exotischen Begleiters dem normalen Stern Gas entziehen und es zu einem Ring um sich selbst formen bevor er es schließlich verschlingt. Wenn das passiert, wird das Material auf über eine Million Grad erhitzt und beginnt Röntgenlicht auszustrahlen.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Si las estrellas están suficientemente cerca entre sí, la fuerte gravedad de la compañera exótica puede arrancar gas de la estrella normal formando un anillo, antes de tragárselo. Cuando esto ocurre, el material se calienta a más de un millón de grados, y empieza a brillar en luz de rayos X.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Als de sterren dichtbij elkaar genoeg staan, kan het exotische object met zijn sterke zwaartekracht gas lostrekken van de normale ster, en het daarna zelf opzuigen. Als dit gebeurt, wordt het gas verhit tot meer dan een miljoen graden en gaat het röntgenstralen uitzenden.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	If the stars are close enough together, the strong gravity of the exotic companion can drag gas off the normal star into a ring itself, before gobbling it up. When this happens the material is heated to over a million degrees and begins shining light as X-rays.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	If the stars are close enough together, the strong gravity of the exotic companion can drag gas off the normal star into a ring itself, before gobbling it up. When this happens the material is heated to over a million degrees and begins shining light as X-rays.

  Razele X dezvăluie găur...  

Show textShow cached sourceOpen source URL	Majoritatea stelelor din Calea Lactee nu sunt solitare, precum este Soarele nostru. 8 din 10 stele masive au una sau mai multe stele ca și companioane. O pereche de stele care orbitează una în jurul celeilalte poartă numele de sistem binar.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Die meisten Sterne unserer Milchstraße schweben nicht wie unsere Sonne allein durch das Weltall. Ein riesiger Anteil der massivsten Sterne, nämlich acht von zehn, haben einen oder mehrere Begleitsterne. Umkreist sich ein Sternenpaar, so nennen wir das ein Doppelsternsystem. Dieses Foto zeigt die auffällige Spiralgalaxie M51. Jeder der so lebendig leuchtenden lilafarbenen Lichtpunkte, die wir auf diesem Bild glitzern sehen, steht für einen besonderen Doppelsternsystemtyp. Wir nennen sie Röntgendoppelsterne, da es sich um Sternenpaare handelt, die Röntgenlicht aussenden.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	La mayoría de las estrellas de la galaxia la Vía Láctea no son como nuestro Sol, que flota solo por el espacio. Hasta 8 de cada 10 de las estrellas más masivas tienen una o más estrellas compañeras. Una pareja de estrellas en órbita una alrededor de la otra recibe el nombre de “sistema binario”. Esta fotografía muestra la majestuosa galaxia espiral llamada Messier 51. Cada punto de vívida luz púrpura que vemos resplandeciendo en esta imagen representa un tipo especial de sistema binario. Les llamamos “binarias de rayos X” porque son parejas de estrellas que resplandecen en luz de rayos X.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	De meeste sterren in de Melkweg zweven niet zoals onze Zon in hun eentje door de ruimte. Acht op de tien zware sterren hebben gezelschap van één of meer sterren. Een paartje sterren dat om elkaar heen draait noemen we een dubbelster. Deze foto laat het flamboyante spiraalvormige sterrenstelsel Messier 51 zien. Elk puntje dat we in levendig paars zien schijnen in dit plaatje is een speciaal soort dubbelster. We noemen ze ‘röntgendubbelsterren’, omdat ze hun licht uitstralen in de vorm van röntgenstraling.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Most of the stars in the Milky Way galaxy are not like our Sun, floating through space alone. A whopping 8-out-of-10 of the most massive stars have one or more companion stars. A pair or stars orbiting each other is called a “binary system”. This photograph shows the flamboyant spiral galaxy called Messier 51. Each point of vivid purple light we are seeing glittering in this picture represents a special type of binary system. We call them ‘X-ray binaries’ because they are pairs of stars shining in X-ray light.

  O fotografie de familie...  

Show textShow cached sourceOpen source URL	Raportat la stele, oamenii există doar de foarte, foarte puțin timp. Stelele trăiesc mii, milioane și chiar miliarde de ani. Prin urmare, este imposibil să urmărim nașterea, viața și moartea aceleași stele, dar putem observa stele diferite aflate în etape diferite ale vieții lor.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Compared to stars, humans have only been around for the blink of an eye. Stars live for thousands, millions or even billions of years. So, we can’t possibly witness the birth, life and death of the same star. However, we can observe stars at different stages of life.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Comparée aux étoiles, l’histoire de l’humanité ne dure pas plus longtemps qu’un clignement d’œil. Par contre, certaines étoiles « vivent » pendant des milliers d’années, d’autres pendant plus de 10 milliards d’années. Nous ne pouvons donc pas être les témoins de la formation d’une étoile jusqu’à ce qu’elle disparaisse. Mais nous pouvons observer les étoiles à différents stades de leur évolution.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Im Vergleich zu Sternen gibt es Menschen erst seit einem Zeitraum eines Wimpernschlags. Sterne leben Tausende, Millionen oder gar Milliarden von Jahren. Daher können wir keinesfalls die Geburt, das Leben und den Tod eines einzelnen Sterns erleben. Allerdings können wir Sterne zu verschiedenen Stadien ihres Lebens beobachten.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Comparados con estrellas, los humanos han existido sólo durante un abrir y cerrar de ojos. Las estrellas viven miles, millones o incluso miles de millones de años. Así que no es posible que podamos ser testigos del nacimiento, vida y muerte de la misma estrella. Sin embargo, podemos observar estrellas en diferentes momentos de la vida.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Rispetto alle stelle, infatti, gli esseri umani hanno una vita lunga appena un battito di ciglia. Le stelle vivono per migliaia, milioni o addirittura miliardi di anni. Di una specifica stella, non possiamo osservare nascita, vita e scomparsa: e tuttavia, possiamo osservare tante stelle diverse, ciascuna in uno stadio differente della propria esistenza.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Em comparação com as estrelas, os seres humanos existem apenas durante um piscar de olhos. As estrelas vivem milhares, milhões ou mesmo milhares de milhões de anos. Portanto, não nos é possível testemunhar o nascimento, a vida e a morte de uma determinada estrela. Podemos contudo observar estrelas em diversos pontos do seu ciclo de vida.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Vergeleken met sterren, bestaat de mensheid korter dan een flits. Sterren leven duizenden, miljoenen of zelfs miljarden jaren lang. Daarom kunnen we onmogelijk zien hoe een enkele ster geboren wordt, leeft en sterft. Maar we kunnen wel sterren bekijken op verschillende momenten van het leven van een ster.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ve srovnání s délkou života hvězd jsou lidé na světě jen mžik, tedy opravdu krátce. Hvězdný život je dlouhý, žijí tisíce, milióny nebo dokonce miliardy let. A my tedy nemůžeme být svědky zrození, života a smrti jedné a té samé hvězdy. Můžeme ale, stejně jako naši mimozemšťané, pozorovat více hvězd v různých fázích jejich života.

  O fotografie de familie...  

Show textShow cached sourceOpen source URL	Raportat la stele, oamenii există doar de foarte, foarte puțin timp. Stelele trăiesc mii, milioane și chiar miliarde de ani. Prin urmare, este imposibil să urmărim nașterea, viața și moartea aceleași stele, dar putem observa stele diferite aflate în etape diferite ale vieții lor.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Compared to stars, humans have only been around for the blink of an eye. Stars live for thousands, millions or even billions of years. So, we can’t possibly witness the birth, life and death of the same star. However, we can observe stars at different stages of life.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Comparée aux étoiles, l’histoire de l’humanité ne dure pas plus longtemps qu’un clignement d’œil. Par contre, certaines étoiles « vivent » pendant des milliers d’années, d’autres pendant plus de 10 milliards d’années. Nous ne pouvons donc pas être les témoins de la formation d’une étoile jusqu’à ce qu’elle disparaisse. Mais nous pouvons observer les étoiles à différents stades de leur évolution.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Im Vergleich zu Sternen gibt es Menschen erst seit einem Zeitraum eines Wimpernschlags. Sterne leben Tausende, Millionen oder gar Milliarden von Jahren. Daher können wir keinesfalls die Geburt, das Leben und den Tod eines einzelnen Sterns erleben. Allerdings können wir Sterne zu verschiedenen Stadien ihres Lebens beobachten.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Comparados con estrellas, los humanos han existido sólo durante un abrir y cerrar de ojos. Las estrellas viven miles, millones o incluso miles de millones de años. Así que no es posible que podamos ser testigos del nacimiento, vida y muerte de la misma estrella. Sin embargo, podemos observar estrellas en diferentes momentos de la vida.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Rispetto alle stelle, infatti, gli esseri umani hanno una vita lunga appena un battito di ciglia. Le stelle vivono per migliaia, milioni o addirittura miliardi di anni. Di una specifica stella, non possiamo osservare nascita, vita e scomparsa: e tuttavia, possiamo osservare tante stelle diverse, ciascuna in uno stadio differente della propria esistenza.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Em comparação com as estrelas, os seres humanos existem apenas durante um piscar de olhos. As estrelas vivem milhares, milhões ou mesmo milhares de milhões de anos. Portanto, não nos é possível testemunhar o nascimento, a vida e a morte de uma determinada estrela. Podemos contudo observar estrelas em diversos pontos do seu ciclo de vida.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Vergeleken met sterren, bestaat de mensheid korter dan een flits. Sterren leven duizenden, miljoenen of zelfs miljarden jaren lang. Daarom kunnen we onmogelijk zien hoe een enkele ster geboren wordt, leeft en sterft. Maar we kunnen wel sterren bekijken op verschillende momenten van het leven van een ster.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ve srovnání s délkou života hvězd jsou lidé na světě jen mžik, tedy opravdu krátce. Hvězdný život je dlouhý, žijí tisíce, milióny nebo dokonce miliardy let. A my tedy nemůžeme být svědky zrození, života a smrti jedné a té samé hvězdy. Můžeme ale, stejně jako naši mimozemšťané, pozorovat více hvězd v různých fázích jejich života.

  O schimbare majoră | Ci...  

Show textShow cached sourceOpen source URL	S-a dovedit că acești misterioși intruși sunt de fapt stele „vagaboande albastre” sau „stele vampir”. Aceste stele vechi au găsit secretul tinereții. Astronomii cred că majoritatea vagaboandelor albastre se formează atunci când două stele orbitează una în jurul celeilalte într-un sistem binar.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	It turns out these mysterious intruders are 'blue stragglers'; old stars that have found the secret to a youthful appearance. Astronomers believe that most blue stragglers form when two stars orbit each other in a binary system. The smaller of the two stars feeds off material from its companion. This provides extra fuel for the smaller star allowing it to burn brighter and bluer, with a fresh young look!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Es hat sich herausgestellt, dass diese geheimnisvollen Eindringlinge “blaue Nachzügler” sind, alte Sterne, die das Geheimnis des jugendlichen Aussehens entdeckt haben. Die Astronomen vermuten, dass sich die meisten der blauen Nachzügler bilden, wenn sich zwei Sterne in einem Doppelsternsystem umkreisen. Der kleiner von beiden ernährt sich von dem Sternenmaterial seines Begleiters. Das bietet zusätzlichen Brennstoff für den kleineren Stern, der es ihm erlaubt, heller und bläulicher zu leuchten, mit einem frischen, jungen Aussehen!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Resulta que estas misteriosas intrusas son 'rezagadas azules' ('blue stragglers' en inglés), estrellas viejas que han encontrado el secreto de una apariencia joven. Los astrónomos piensan que la mayoría de 'rezagadas azules' se forma cuando dos estrellas están en órbita una alrededor de la otra en un sistema binario. La más pequeña de las dos estrellas se alimenta de material de su compañera. Esto proporciona combustible extra para la estrella más pequeña, permitiéndole brillar más intensamente y más azul, ¡con un fresco aspecto joven!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Il punto è che questi intrusi misteriosi sono "blue stragglers" (in italiano "stelle vagabonde blu"), stelle vecchie che hanno scoperto il segreto per sembrare giovani. Gli astronomi pensano che la maggior parte di queste blue stragglers si formi quando due stelle orbitano una attorno all'altra in un sistema binario. La stella più piccola ruba materiale alla compagna, e la dose extra di combustibile le permette di brillare più intensamente e con un colore più blu, dandole un aspetto così giovane!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Verifica-se que estes misteriosos intrusos são 'retardatários azuis'; estrelas antigas que descobriram o segredo para uma aparência jovem. Os astrónomos acreditam que os retardatários mais azuis resultam de duas estrelas que orbitam entre si num sistema binário. A estrela menor alimenta-se da sua companheira que lhe fornece combustível extra permitindo-lhe ser mais brilhante e queimar com uma cor mais azul, com um olhar fresco e jovem!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Het blijken blauwe 'nakomers' te zijn: oude sterren die erin zijn geslaagd jong over te komen. De nakomers worden gevormd wanneer twee sterren in een dubbelstersysteem om elkaar heen draaien. De kleinere van de twee pakt materiaal af van zijn begeleider. Daardoor heeft de ster extra brandstof en schijnt hij blauwer en helderder, als een jonge ster!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	It turns out these mysterious intruders are 'blue stragglers'; old stars that have found the secret to a youthful appearance. Astronomers believe that most blue stragglers form when two stars orbit each other in a binary system. The smaller of the two stars feeds off material from its companion. This provides extra fuel for the smaller star allowing it to burn brighter and bluer, with a fresh young look!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Okazuje się, że te gwiazdy nazywane „błękitnymi maruderami” mimo swego starego wieku odkryły tajemnice wiecznej młodości. Astronomowie przypuszczają, że takie obiekty tworzą się, kiedy dwie gwiazdy krążą wokół siebie tworząc gwiazdę podwójną. Mniejsza z gwiazd układu ściąga otoczkę gwiazdową ze swego kompana, pozyskując w ten sposób więcej paliwa, co pozwala jej na wolniejsze starzenie – jest więc bardziej niebieska i gorąca.

  O schimbare majoră | Ci...  

Show textShow cached sourceOpen source URL	S-a dovedit că acești misterioși intruși sunt de fapt stele „vagaboande albastre” sau „stele vampir”. Aceste stele vechi au găsit secretul tinereții. Astronomii cred că majoritatea vagaboandelor albastre se formează atunci când două stele orbitează una în jurul celeilalte într-un sistem binar.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	It turns out these mysterious intruders are 'blue stragglers'; old stars that have found the secret to a youthful appearance. Astronomers believe that most blue stragglers form when two stars orbit each other in a binary system. The smaller of the two stars feeds off material from its companion. This provides extra fuel for the smaller star allowing it to burn brighter and bluer, with a fresh young look!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Es hat sich herausgestellt, dass diese geheimnisvollen Eindringlinge “blaue Nachzügler” sind, alte Sterne, die das Geheimnis des jugendlichen Aussehens entdeckt haben. Die Astronomen vermuten, dass sich die meisten der blauen Nachzügler bilden, wenn sich zwei Sterne in einem Doppelsternsystem umkreisen. Der kleiner von beiden ernährt sich von dem Sternenmaterial seines Begleiters. Das bietet zusätzlichen Brennstoff für den kleineren Stern, der es ihm erlaubt, heller und bläulicher zu leuchten, mit einem frischen, jungen Aussehen!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Resulta que estas misteriosas intrusas son 'rezagadas azules' ('blue stragglers' en inglés), estrellas viejas que han encontrado el secreto de una apariencia joven. Los astrónomos piensan que la mayoría de 'rezagadas azules' se forma cuando dos estrellas están en órbita una alrededor de la otra en un sistema binario. La más pequeña de las dos estrellas se alimenta de material de su compañera. Esto proporciona combustible extra para la estrella más pequeña, permitiéndole brillar más intensamente y más azul, ¡con un fresco aspecto joven!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Il punto è che questi intrusi misteriosi sono "blue stragglers" (in italiano "stelle vagabonde blu"), stelle vecchie che hanno scoperto il segreto per sembrare giovani. Gli astronomi pensano che la maggior parte di queste blue stragglers si formi quando due stelle orbitano una attorno all'altra in un sistema binario. La stella più piccola ruba materiale alla compagna, e la dose extra di combustibile le permette di brillare più intensamente e con un colore più blu, dandole un aspetto così giovane!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Verifica-se que estes misteriosos intrusos são 'retardatários azuis'; estrelas antigas que descobriram o segredo para uma aparência jovem. Os astrónomos acreditam que os retardatários mais azuis resultam de duas estrelas que orbitam entre si num sistema binário. A estrela menor alimenta-se da sua companheira que lhe fornece combustível extra permitindo-lhe ser mais brilhante e queimar com uma cor mais azul, com um olhar fresco e jovem!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Het blijken blauwe 'nakomers' te zijn: oude sterren die erin zijn geslaagd jong over te komen. De nakomers worden gevormd wanneer twee sterren in een dubbelstersysteem om elkaar heen draaien. De kleinere van de twee pakt materiaal af van zijn begeleider. Daardoor heeft de ster extra brandstof en schijnt hij blauwer en helderder, als een jonge ster!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	It turns out these mysterious intruders are 'blue stragglers'; old stars that have found the secret to a youthful appearance. Astronomers believe that most blue stragglers form when two stars orbit each other in a binary system. The smaller of the two stars feeds off material from its companion. This provides extra fuel for the smaller star allowing it to burn brighter and bluer, with a fresh young look!
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Okazuje się, że te gwiazdy nazywane „błękitnymi maruderami” mimo swego starego wieku odkryły tajemnice wiecznej młodości. Astronomowie przypuszczają, że takie obiekty tworzą się, kiedy dwie gwiazdy krążą wokół siebie tworząc gwiazdę podwójną. Mniejsza z gwiazd układu ściąga otoczkę gwiazdową ze swego kompana, pozyskując w ten sposób więcej paliwa, co pozwala jej na wolniejsze starzenie – jest więc bardziej niebieska i gorąca.

  O schimbare majoră | Ci...  

Show textShow cached sourceOpen source URL	Astfel, putem presupune că stelele albastre sunt prin comparație mai tinere. Stelele albastre ard foarte intens fiind foarte luminoase și fierbinți, lucru care duce la un consum ridicat de energie. Ele își consumă combustibilul foarte repede și nu trăiesc la fel de mult ca stelele puțin vizibile.
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Likewise, we can assume blue stars are comparatively young. This is because blue stars burn very bright and hot which takes a lot of energy, so they consume their fuel very quickly and don't live as long as dimmer stars. Surprisingly, there are quite a few blue stars in this cluster. If they formed 10 billion years ago with the rest of the stars, they should have fizzled out long before now. How did they survive?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Ebenso könne wir davon ausgehen, dass blaue Sterne vergleichsweise jung sind. Das liegt daran, dass blaue Sterne sehr hell leuchten und auch sehr heiß sind. Sie verbrauchen ihren Brennstoff sehr schnell und leben somit nicht so lange wie dunklere Sterne. Erstaunlicherweise befinden sich in diesem Kugelsternhaufen durchaus ein paar blaue Sterne. Wenn sie wirklich zusammen mit den anderen Sternen vor 10 Milliarden Jahren gebildet wurden, sollten sie eigentlich längst verschwunden sein. Wie haben sie überlebt?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	De forma similar, podemos asumir que las estrellas azules son jóvenes en comparación. Esto es porque las estrellas azules son muy brillantes y calientes, lo que quita mucha energía, así que consumen su combustible muy rápidamente y no viven tanto como las estrellas menos brillantes. Sorprendentemente, hay unas cuantas estrellas azules en este cúmulo. Si se formaron hace 10 mil millones de años junto con el resto de estrellas, deberían de haberse apagado hace mucho tiempo. ¿Cómo sobrevivieron?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Invece, si pensa che le stelle blu siano piuttosto giovani. Infatti, le stelle blu bruciano in maniera molto intensa e molto calda, consumando tantissima energia velocemente, e quindi non vivono tanto quanto le stelle più fioche. Sorprendentemente, ci sono diverse stelle blu in quest'ammasso. Se queste stelle blu si fossero formate 10 miliardi di anni fa, insieme al resto delle stelle, a quest'ora sarebbero spente da molto tempo. Come sono riuscite a sopravvivere?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Da mesma forma, podemos supor que as estrelas azuis são relativamente jovens. Isto é porque as estrelas azuis são muito quentes e brilhantes consumindo muita energia e queimando o seu combustível muito rapidamente. Vivem assim menos tempo do que as estrelas de menor brilho. Surpreendentemente, existem algumas estrelas azuis no aglomerado. Se elas se formaram há 10 milhares de milhões de anos atrás como as restantes estrelas, deveriam ter envelhecido há muito tempo. Como sobreviveram?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Blauwe sterren zijn relatief jong. Dat komt doordat blauwe sterren heel helder en heet stralen, wat veel energie kost. Ze verbruiken hun brandstof erg snel en leven niet zo lang als zwakkere sterren. Er zijn op de foto best veel blauwe sterren te zien. Wanneer die 10 miljard jaar geleden gevormd zijn, tegelijk met de andere sterren, zouden ze al lang zijn opgebrand. Hoe hebben ze kunnen overleven?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Likewise, we can assume blue stars are comparatively young. This is because blue stars burn very bright and hot which takes a lot of energy, so they consume their fuel very quickly and don't live as long as dimmer stars. Surprisingly, there are quite a few blue stars in this cluster. If they formed 10 billion years ago with the rest of the stars, they should have fizzled out long before now. How did they survive?
Compare text pagesCompare HTM pagesOpen source URLOpen target URLDefine space-awareness.org as primary domain	Możemy też założyć, że niebieskie gwiazdy są stosunkowo młode. Dzieje się tak dlatego, że niebieskie gwiazdy są dość gorące i jasne, więc tracą sporo energii i swego paliwa, którego brak nie pozwala im na dłuższe życie jak w przypadku słabszych chłodniejszych gwiazd. O dziwo, na prezentowanym zdjęciu można odnaleźć również i niebieskie gwiazdy. Jeśli powstały tak jak reszta gwiazd w gromadzie 10 miliardów lat temu powinny już dawno zakończyć swój żywot. Jak przetrwały?