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АгӀонан чулацам кхечу меттанашкахь тӀекхочуш бац.
ХӀара агӀо Википеди чуьра йу — маьрша энциклопеди

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ХӀара файл Викиларма чуьра йу и лело йиш йу массо проекташкахь. Цунна хаам гайтина лахахь. Файл Викилармехь

Файлах лаьцна

Википеди

 ХӀокху файлан ю хаьржина суьртан статус (Seçkin resimler) Википедехь (турецкий раздел) и хӀинца дикачеран суьртийн юкъахь ду.

Хьайна хӀокху файлан Виикигуламехь «хаьржина» статус йогӀу аьлла хитахь эхь ца хеташ кховдаде и.
Хьайгахь маьрша лицензица чудакха йиш йолуш хӀара сана дика сурт делахь, дехар до, чудаккха иза, харжа лицензи и кховдаде иза.

Цуьнах лаьцна
English: Eskimo nebula (NGC 2392). In its first glimpse of the heavens following the successful December 1999 servicing mission, NASA's Hubble Space Telescope captured a majestic view of a planetary nebula, the glowing remains of a dying, Sun-like star. This stellar relic, first spied by William Herschel in 1787, is nicknamed the "Eskimo" Nebula (NGC 2392) because, when viewed through ground-based telescopes, it resembles a face surrounded by a fur parka.

In this Hubble telescope image, the "parka" is really a disk of material embellished with a ring of comet-shaped objects, with their tails streaming away from the central, dying star. The Eskimo's "face" also contains some fascinating details. Although this bright central region resembles a ball of twine, it is, in reality, a bubble of material being blown into space by the central star's intense "wind" of high-speed material.

In this photo, one bubble lies in front of the other, obscuring part of the second lobe. Scientists believe that a ring of dense material around the star's equator, ejected during its red giant phase, created the nebula's shape. The bubbles are not smooth like balloons but have filaments of denser matter. Each bubble is about 1 light-year long and about half a light-year wide.

Scientists are still puzzled about the origin of the comet-shaped features in the "parka." One possible explanation is that these objects formed from a collision of slow-and fast-moving gases.

The Eskimo Nebula is more than 2,870 light-years from Earth in the constellation Gemini. The picture was taken Jan. 10 and 11, 2000, with the Wide Field and Planetary Camera 2. The nebula's glowing gases produce the colors in this image: nitrogen (red), hydrogen (green), oxygen (blue), and helium (violet).
Терахь
Хьост http://www.spacetelescope.org/images/heic9910a/
Автор NASA, ESA, Andrew Fruchter (STScI), and the ERO team (STScI + ST-ECF)
Бакъонаш
(Йуха хӀара файл лелор)
Public domain
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.
Кхин версеш Derivative works of this file:  EvolutionSystèmeSolaire-fragment1.png

Куьг

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Файлан истори

Тlетаlаде терахь/хан, муха хилла хьажарна и файл.

Терахь/ХанЖимаФайлан барамДекъашхоБилгалдаккхар
карара2005, 28 июль, 12:34Жимо верси 2005, 28 июль, 12:341500 × 1500 (1,16 Мб)Startaq
2005, 1 февраль, 17:20Жимо верси 2005, 1 февраль, 17:20320 × 259 (12 Кб)CWitteEskimo nebula

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