by APOD Robot » Thu Jan 21, 2021 5:09 am
M78 Wide Field
Explanation: Interstellar dust clouds and
glowing nebulae abound in the fertile
constellation of Orion. One of the
brightest, M78, is centered in this colorful,
wide field view, covering an area north of
Orion's belt. At a distance of about 1,500 light-years, the bluish reflection nebula is around 5 light-years across. Its tint is due to dust
preferentially reflecting the
blue light of hot, young stars. Reflection nebula NGC 2071 is
just to the left of M78. Flecks of emission from
Herbig-Haro objects, energetic jets from stars in the process of formation, stand out against the dark dust lanes. The exposure also brings out the region's fainter, pervasive reddish glow of atomic hydrogen gas.
[url=https://apod.nasa.gov/apod/ap210121.html] [img]https://apod.nasa.gov/apod/calendar/S_210121.jpg[/img] [size=150]M78 Wide Field[/size][/url]
[b] Explanation: [/b] [url=http://www-ssg.sr.unh.edu/ism/what1.html]Interstellar[/url] dust clouds and [url=https://nasaviz.gsfc.nasa.gov/12086]glowing nebulae[/url] abound in the fertile [url=https://apod.nasa.gov/apod/ap161204.html]constellation of Orion[/url]. One of the [url=http://www.messier.seds.org/m/m078.html]brightest, M78[/url], is centered in this colorful, [url=https://www.astrobin.com/wj6sox/?nc=user]wide field view[/url], covering an area north of [url=https://apod.nasa.gov/apod/ap171123.html]Orion's belt[/url]. At a distance of about 1,500 light-years, the bluish reflection nebula is around 5 light-years across. Its tint is due to dust [url=http://leo.astronomy.cz/mix/mix.html]preferentially[/url] reflecting the [url=http://math.ucr.edu/home/baez/physics/General/BlueSky/blue_sky.html]blue light[/url] of hot, young stars. Reflection nebula NGC 2071 is [url=http://www.starpointing.com/ccd/m78_labeled.html]just to the left[/url] of M78. Flecks of emission from [url=https://en.wikipedia.org/wiki/Herbig%E2%80%93Haro_object#Discovery_and_history_of_observations]Herbig-Haro objects[/url], energetic jets from stars in the process of formation, stand out against the dark dust lanes. The exposure also brings out the region's fainter, pervasive reddish glow of atomic hydrogen gas.
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