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Keywords: Orion Nebula, star formation, molecular cloud, infrared
![M16 крупным планом](https://images.astronet.ru/pubd/2019/08/11/0001490195/M16_HSHO_crop2_1024.preview.jpg)
10.08.2019
A star cluster around 2 million years young surrounded by natal clouds of dust and glowing gas, M16 is also known as The Eagle Nebula. This beautifully detailed image of the region adopts the colorful Hubble palette and includes cosmic sculptures made famous in Hubble Space Telescope close-ups of the starforming complex.
![Темный Морской конек в Цефее](https://images.astronet.ru/pubd/2019/10/24/0001519507/Barnard150Seahorse1024.preview.jpg)
24.10.2019
Light-years across, this suggestive shape known as the Seahorse Nebula appears in silhouette against a rich, luminous background of stars. Seen toward the royal northern constellation of Cepheus, the dusty, obscuring clouds are part of a Milky Way molecular cloud some 1,200 light-years distant.
![Темный Морской конек в Цефее](https://images.astronet.ru/pubd/2021/11/05/0001781347/b150_avitabile1092c.preview.jpg)
5.11.2021
Light-years across, this suggestive shape known as the Seahorse Nebula appears in silhouette against a rich, luminous background of stars. Seen toward the royal northern constellation of Cepheus, the dusty, obscuring clouds are part of a Milky Way molecular cloud some 1,200 light-years distant.
![Туманность Северная Америка в инфракрасном свете](https://images.astronet.ru/pubd/2019/07/28/0001486288/northamerica_ir_960.preview.jpg)
28.07.2019
The North America Nebula can do what most North Americans cannot -- form stars. Precisely where in the nebula these stars are forming has been mostly obscured by some of the nebula's thick dust that is opaque to visible light.
![Туманность Ориона в телескоп "Спитцер"](https://images.astronet.ru/pubd/2019/09/03/0001494900/orion2010_spitzerMedRC.preview.jpg)
31.08.2019
Few cosmic vistas excite the imagination like the Orion Nebula, an immense stellar nursery some 1,500 light-years away. Spanning about 40 light-years across the region, this infrared image from the Spitzer Space Telescope...
![К югу от Ориона](https://images.astronet.ru/pubd/2022/01/27/0001806629/NGC-1999_1100.preview.jpg)
27.01.2022
South of the large star-forming region known as the Orion Nebula, lies bright blue reflection nebula NGC 1999. At the edge of the Orion molecular cloud complex some 1,500 light-years distant, NGC 1999's illumination is provided by the embedded variable star V380 Orionis.
![NGC 1893 и Головастики в IC 410](https://images.astronet.ru/pubd/2024/02/02/0001919424/Tadpoles1024original.preview.png)
2.02.2024
This cosmic view shows off an otherwise faint emission nebula IC 410, captured under clear Netherlands skies with telescope and narrowband filters. Above and right of center you can spot two remarkable inhabitants of the interstellar pond of gas and dust, known as the tadpoles of IC 410.
![Когда розы не красные](https://images.astronet.ru/pubd/2018/02/22/0001399069/RosetteNebulaNBHColesHelm1024.preview.jpg)
22.02.2018
Not all roses are red of course, but they can still be very pretty. Likewise, the beautiful Rosette Nebula and other star forming regions are often shown in astronomical images with a predominately red hue, in part because the dominant emission in the nebula is from hydrogen atoms.
![В сердце Ориона](https://images.astronet.ru/pubd/2015/01/02/0001329560/TrapeziumCluster_Francsics_apod1024.preview.jpg)
1.01.2015
Near the center of this sharp cosmic portrait, at the heart of the Orion Nebula, are four hot, massive stars known as the Trapezium. Tightly gathered within a region about 1.5 light-years in radius, they dominate the core of the dense Orion Nebula Star Cluster.
![Трапеция: в сердце Ориона](https://images.astronet.ru/pubd/2024/01/07/0001916530/Image964_1024.preview.jpg)
5.01.2024
Near the center of this sharp cosmic portrait, at the heart of the Orion Nebula, are four hot, massive stars known as the Trapezium. Gathered within a region about 1.5 light-years in radius, they dominate the core of the dense Orion Nebula Star Cluster.
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