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Keywords: Spitzer space telescope, star formation, Eta Carinae, nebula, dust, infrared
![Трехраздельная туманность](https://images.astronet.ru/pubd/2003/09/08/0001192773/m20castano_block_c1.preview.jpg)
1.09.2003
The beautiful Trifid Nebula (aka M20), a photogenic study in cosmic contrasts, lies about 5,000 light-years away toward the nebula rich constellation Sagittarius. A star forming region in the plane of our galaxy...
![NGC 1579: северная Трехраздельная туманность](https://images.astronet.ru/pubd/2006/05/26/0001214295/ngc1579_gabany_c55.preview.jpg)
25.05.2006
Colorful NGC 1579 resembles the better known Trifid Nebula, but lies much farther north in planet Earth's sky, in the heroic constellation Perseus. About 2,100 light-years away and 3 light-years across, NGC 1579 is a captivating study in color.
![Прекрасная Трехраздельная туманность](https://images.astronet.ru/pubd/2005/05/26/0001206070/m20_jacobsen_f41.preview.jpg)
26.05.2005
The beautiful Trifid Nebula (aka M20), a photogenic study in cosmic contrasts, lies about 5,000 light-years away toward the nebula rich constellation Sagittarius. A star forming region in the plane of our galaxy...
![Трехраздельная туманность: вид в канадско-французский телескоп на Гавайях](https://images.astronet.ru/pubd/2005/05/31/0001206118/m20_cfht.preview.jpg)
31.05.2005
Unspeakable beauty and unimaginable bedlam can be found together in the Trifid Nebula. Also known as M20, this photogenic nebula is visible with good binoculars towards the constellation of Sagittarius. The energetic processes of star formation create not only the colors but the chaos. The red-glowing gas results from high-energy starlight striking interstellar hydrogen gas.
![Инфракрасные наблюдения Юпитера](https://images.astronet.ru/pubd/2003/03/13/0001187628/jupiter_wiro8_full.preview.jpg)
13.03.2003
Gazing out over the mountaintops from the Wyoming InfraRed Observatory (WIRO), astronomers recently recorded this bizarre looking image of the solar system's ruling planet, gas giant Jupiter. The false-color picture is a composite...
![NGC 253: галактика в созвездии Скульптор](https://images.astronet.ru/pubd/2004/08/14/0001199193/ngc253_hst_big.preview.jpg)
9.12.1998
NGC 253 is not only one of the brightest spiral galaxies visible, it is also one of the dustiest. Discovered in 1783 by Caroline Herschel in the constellation of Sculptor, NGC 253 lies only about ten million light-years distant.
![Когда розы не красные](https://images.astronet.ru/pubd/2006/03/24/0001212565/Rosette_ballauer_640.preview.jpg)
24.03.2006
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.
![LL Ориона и туманность Ориона](https://images.astronet.ru/pubd/2006/01/21/0001211023/llori_orion_hst_c14.preview.jpg)
20.01.2006
This esthetic close-up of cosmic clouds and stellar winds features LL Orionis, interacting with the Orion Nebula flow. Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun.
![Туманность Ориона. Вид в телескоп Хаббла](https://images.astronet.ru/pubd/2006/01/21/0001211024/m42_hst_c45.preview.jpg)
19.01.2006
Few cosmic vistas excite the imagination like the Orion Nebula. Also known as M42, the nebula's glowing gas surrounds hot young stars at the edge of an immense interstellar molecular cloud only 1,500 light-years away.
![Игра в "скорлупки" в БМО](https://images.astronet.ru/pubd/2006/05/18/0001214159/lmc_gleason_f23.preview.jpg)
18.05.2006
An alluring sight in dark southern skies, the Large Magellanic Cloud (LMC) is seen here through a narrow filter that transmits only the red light of hydrogen atoms. Ionized by energetic starlight, a hydrogen atom emits the characteristic red H-alpha light as its single electron is recaptured and transitions to lower energy states.
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