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This photo of the Horsehead nebula was captured by NASA’s Hubble Telescope in infrared. It’s located in the constellation Orion about 1,500 light years away from us.

This photo of the Horsehead nebula was captured by NASA’s Hubble Telescope in infrared. It’s located in the constellation Orion about 1,500 light years away from us.

Images taken of land masses (Earth at Night) by  . . . . geostationary satellites using long term exposure

Earth at Night

Images taken of land masses (Earth at Night) by . . . . geostationary satellites using long term exposure

The image shows the central region of the Tarantula Nebula in the Large Magellanic Cloud. The young and dense star cluster R136 can be seen at the lower right of the image. This cluster contains hundreds of young blue stars, among them the most massive star detected in the Universe so far. Using the NASA/ESA Hubble Space Telescope astronomers were able to study the central and most dense region of this cluster in detail. Here they found nine stars with more than 100 solar masses.

Le télescope Hubble saisit une pouponnière d’étoiles mastodontes

The image shows the central region of the Tarantula Nebula in the Large Magellanic Cloud. The young and dense star cluster R136 can be seen at the lower right of the image. This cluster contains hundreds of young blue stars, among them the most massive star detected in the Universe so far. Using the NASA/ESA Hubble Space Telescope astronomers were able to study the central and most dense region of this cluster in detail. Here they found nine stars with more than 100 solar masses.

man, stuck in infinity. the abyss.

man, stuck in infinity. the abyss.

A spectacular Hubble Space Telescope image reveals the heart of the Lagoon Nebula. Seen as a massive cloud of glowing dust and gas, bombarded by the energetic radiation of new stars, this placid name hides a dramatic reality.

A spectacular Hubble Space Telescope image reveals the heart of the Lagoon Nebula. Seen as a massive cloud of glowing dust and gas, bombarded by the energetic radiation of new stars, this placid name hides a dramatic reality.

Inside the #CarinaNebula: Cropped from original 465 mb tif image. A towering “mountain” of cold hydrogen gas laced with dust is the site of new star formation in the Carina Nebula (NGC 3372). The great gas pillar is being eroded by the ultraviolet radiation from the hottest newborn stars in the nebula. This portion of the Carina Nebula is home to some of the most intense star formation in the Milky Way galaxy. Credit: NASA/Hubble

Inside the #CarinaNebula: Cropped from original 465 mb tif image. A towering “mountain” of cold hydrogen gas laced with dust is the site of new star formation in the Carina Nebula (NGC 3372). The great gas pillar is being eroded by the ultraviolet radiation from the hottest newborn stars in the nebula. This portion of the Carina Nebula is home to some of the most intense star formation in the Milky Way galaxy. Credit: NASA/Hubble

PHOTOS. Hubble 2010 : Piliers de la Création dans Carène

PHOTOS. Hubble a 25 ans : voici ses plus beaux clichés du cosmos

PHOTOS. Hubble 2010 : Piliers de la Création dans Carène

La Nébuleuse de la Tête de Cheval vue en infra-rouge (source #NASA)

La Nébuleuse de la Tête de Cheval vue en infra-rouge (source #NASA)

The Elephant’s Trunk nebula in 3D. | 32 Mesmerising GIFs That Will Make You Fall In Love With Science

The Elephant's Trunk nebula in 3D.

The Elephant’s Trunk nebula in 3D. | 32 Mesmerising GIFs That Will Make You Fall In Love With Science

Horsehead Nebula. (La Nebulosa Testa di Cavallo, nota anche come Barnard 33, B33 , è una nebulosa oscura nella costellazione di Orione. La Nebulosa è una regione di gas più densa del mezzo circostante in via di disgregazione a causa dell'intensa radiazione ultravioletta di stelle come σ Orionis. Secondo uno dei modelli ipotizzati  sarebbe in uno stadio iniziale del processo che porterà alla formazione di un globulo di Bok.)

Horsehead Nebula. (La Nebulosa Testa di Cavallo, nota anche come Barnard 33, B33 , è una nebulosa oscura nella costellazione di Orione. La Nebulosa è una regione di gas più densa del mezzo circostante in via di disgregazione a causa dell'intensa radiazione ultravioletta di stelle come σ Orionis. Secondo uno dei modelli ipotizzati sarebbe in uno stadio iniziale del processo che porterà alla formazione di un globulo di Bok.)

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