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You entered: tail
![Звездное скопление за хвостом кометы Хейла-Боппа](https://images.astronet.ru/pubd/2003/06/23/0001191163/halebopp8_aac_big.preview.jpg)
16.04.1997
Comet Hale-Bopp continues to look impressive. The photograph above captured the comet on April 7th passing nearly in front of M34, a star cluster in the constellation of Perseus. Many of the stars in this open cluster can be seen through Comet Hale-Bopp's white dust tail.
![Два хвоста кометы Веста](https://images.astronet.ru/pubd/2002/08/20/0001178965/comet_west.preview.gif)
26.08.1995
Here Comet West is seen showing two enormous tails that wrap around the sky. The ion tale of a comet usually appears more blue and always points away from the Sun. The dust tail trailing the comet's nucleus is the most prominent.
![Комета Хиякутаке: звезды через хвост](https://images.astronet.ru/pubd/2004/03/22/0001197228/hyakutake_scott_big.preview.jpg)
17.07.1998
Comets are cosmic icebergs. They follow very elongated orbits which carry them from the frozen, remote outer reaches of the Solar System to close encounters with the Sun. Heated by sunlight, they slough off layers of material as gas and dust, forming their characteristic awe-inspiring comas (heads) and tails.
![Развивающиеся хвосты кометы Хейла-Боппа](https://images.astronet.ru/pubd/2003/06/22/0001191123/halebopp4_aac.preview.jpg)
14.03.1997
Comet Hale-Bopp is living up to its expectations. Besides the brightness of its coma, a comet is typically remembered by the length of its tails. As visible in the above picture taken last week, Comet Hale-Bopp's blue ion tail shows a dramatic extension, with current reports of about 20 degrees from dark locations.
![Длинный хвост кометы Леонарда](https://images.astronet.ru/pubd/2022/01/03/0001799038/LeonardTail_Hattenbach_960.preview.jpg)
3.01.2022
You couldn't see Comet LeonardБs extremely long tail with a telescope Б it was just too long. You also couldn't see it with binoculars Б still too long. Or with your eyes -- it was too dim. Or from a city Б the sky was too bright.
![Переменный ионный хвост кометы Хейла-Боппа](https://images.astronet.ru/pubd/2003/06/23/0001191195/halebopp9_aac_big.preview.jpg)
14.05.1997
What's happening to Comet Hale-Bopp's blue ion tail? The comet's ion tail is fluctuating more rapidly as it passes a region of changing solar wind. As the comet passes from north to south, it crosses the plane of the Sun's equator, where the solar magnetic field changes direction.
![Хвост кометы над горизонтом](https://images.astronet.ru/pubd/2007/01/24/0001220475/naughtail_fulle.preview.jpg)
24.01.2007
What's happening over the horizon? Many a sky enthusiast who thought they had seen it all had never seen anything like this. To the surprise of many Northern Hemisphere observers, the tail of Comet McNaught remained visible even after the comet's head set ahead of the Sun.
![Комета Икея-Жанга виляет хвостом](https://images.astronet.ru/pubd/2002/05/15/0001176820/cometiz_karrer.preview.gif)
15.05.2002
As Comet Ikeya-Zhang approached the Sun two months ago, it developed a complex blue ion tail. The tail was composed of ions that boiled off the nucleus and were pushed away from the Sun by the out-flowing fast-moving particles of the solar wind.
![Длинный хвост кометы SWAN](https://images.astronet.ru/pubd/2020/05/08/0001653615/c2020_f8_2020_05_02dp_1024.preview.jpg)
8.05.2020
Blowing in the solar wind the spectacular ion tail of Comet SWAN (C/2020 F8) extends far across this 10 degree wide telephoto field of view. Captured on May 2 its greenish coma was about 6 light-minutes from Earth. The pretty background starfield lies near the border of the constellations Cetus and Aquarius.
![Анти-хвост кометы ПанСТАРРС](https://images.astronet.ru/pubd/2013/05/19/0001287737/panstarrs15may2013-mfulle_1368632878_1000.preview.jpg)
18.05.2013
Once the famous sunset comet, PanSTARRS (C/2011 L4) is now visible all night from much of the northern hemisphere, bound for the outer solar system as it climbs high above the ecliptic plane. Dimmer and fading, the comet's broad dust tail is still growing, though.
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