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You entered: hydrogen
![Спектр вспышки Солнца](https://images.astronet.ru/pubd/2013/11/15/0001295821/emmanouilidi200mmFlashSpect950.preview.jpg)
15.11.2013
In a flash, the visible spectrum of the Sun changed from absorption to emission on November 3rd, during the brief total phase of a solar eclipse. That fleeting moment is captured by telephoto lens and diffraction grating in this well-timed image from clearing skies over Gabon in equatorial Africa.
![Колыбель в Орионе](https://images.astronet.ru/pubd/2007/01/25/0001220493/orioncradle_hallas_r780.preview.jpg)
25.01.2007
Cradled in glowing hydrogen, stellar nurseries in Orion lie at the edge of a giant molecular cloud some 1,500 light-years away. This breath-taking view spans about 13 degrees across the center of the well-known constellation with the Great Orion Nebula, the closest large star forming region, just right of center.
![Хиякутаке: атмосфера кометы](https://images.astronet.ru/pubd/2003/09/08/0001192808/hyakutake1_hst_big.preview.gif)
10.04.1998
The atmosphere of a comet comes and goes. Approaching the sun, it swells as material from the icy cometary nucleus is warmed and evaporated by increasing sunlight. Immense but tenuous and fleeting, the inner atmosphere or inner "coma" of comet Hyakutake is seen in this false color picture.
![IC 1396 крупным планом](https://images.astronet.ru/pubd/2005/09/30/0001208268/ic1396b_wright_f13.preview.jpg)
30.09.2005
Clouds of glowing hydrogen gas mingle ominously with dark dust lanes in this close-up of IC 1396, an active star forming region some 2,000 light years away in the constellation Cepheus. In this and other similar emission nebulae, energetic ultraviolet light from a hot young star strips electrons from the surrounding hydrogen atoms.
![Извержение на Солнце](https://images.astronet.ru/pubd/2002/08/20/0001178936/sun_skylab.preview.gif)
13.08.1995
The sun was captured in 1973 throwing one of the largest eruptive prominences ever recorded. Sol, our sun, is a normal star. It formed about 5 billion years ago, and will last about another 5 billion years. The sun will never explode, and a solar flare will never destroy the earth.
![Игра в скорлупки в БМО](https://images.astronet.ru/pubd/2016/12/30/0001373677/lmcapodgleason960.preview.jpg)
29.12.2016
An alluring sight in southern skies, the Large Magellanic Cloud (LMC) is seen here through narrowband filters. The filters are designed to transmit only light emitted by ionized sulfur, hydrogen, and oxygen atoms. Ionized...
![Облака на Юпитере](https://images.astronet.ru/pubd/2003/08/15/0001192352/jupclouds_vgr_big.preview.jpg)
20.09.1997
What makes the colors in Jupiter's clouds? With a mean temperature of 120 degrees Kelvin (-153 degrees Celsius) and a composition dominated by hydrogen (about 90%), and helium (about 10%) with a smattering...
![Спектр вспышки Солнца](https://images.astronet.ru/pubd/2016/03/12/0001358191/tse2016FulhamP3090040_1065c.preview.jpg)
12.03.2016
In a flash, the visible spectrum of the Sun changed from absorption to emission on March 9 during the total solar eclipse. That fleeting moment, at the beginning the total eclipse phase, is captured by telephoto lens and diffraction grating in this image from clearing skies over Ternate, Indonesia.
![Разноцветные облака на Юпитере](https://images.astronet.ru/pubd/2007/04/08/0001221486/jupclouds_vgr_big.preview.jpg)
3.08.1996
What makes the colors in Jupiter's clouds? With a mean temperature of 120 degrees Kelvin (-153 degrees Celsius) and a composition dominated by Hydrogen (about 90%), and Helium (about 10%) with a smattering...
![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.
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