Fayl:NGC3895 - HST - Potw2021a.tif

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One Large Stellar Latte To Go


Far away in the Ursa Major constellation is a swirling galaxy that would not look out of place on a coffee made by a starry-eyed barista. NGC 3895 is a barred spiral galaxy that was first spotted by William Herschel in 1790 and was later observed by the NASA/ESA Hubble Space Telescope.

Hubble's orbit high above the Earth's distorting atmosphere allows astronomers to make the very high resolution observations that are essential to opening new windows on planets, stars and galaxies — such as this beautiful view of NGC 3895. The telescope is positioned approximately 570 km above the ground, where it whirls around Earth at 28 000 kilometres per hour and takes 96 minutes to complete one orbit.

Credit:

ESA/Hubble, NASA, and R. Barrows 


Coordinates
Position (RA):  	11 49 4.01
Position (Dec): 	59° 25' 57.40"
Field of view:  	0.68 x 0.67 arcminutes
Orientation:    	North is 46.4° right of vertical

Colours & filters Band	Wavelength	Telescope
Optical B       	438 nm	Hubble Space Telescope WFC3
Optical I       	814 nm	Hubble Space Telescope WFC3
Infrared H      	1.6 μm	Hubble Space Telescope WFC3
.
Sanasi 25 May 2020, 06:00 (Release)
Manba https://spacetelescope.org/images/potw2021a/ https://spacetelescope.org/static/archives/images/original/potw2021a.tif
Muallif Credit: ESA/Hubble, NASA, and R. Barrows
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This file is licensed under the Creative Commons Attribution 4.0 International license.
Attributsiya: ESA/Hubble
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joriy07:19, 25-May 202007:19, 25-May 2020 dagi versiya uchun tasvir1 025 × 1 014 (5,98 MB)Fabian RRRR== {{int:filedesc}} == {{Information |Description='''One Large Stellar Latte To Go Far away in the Ursa Major constellation is a swirling galaxy that would not look out of place on a coffee made by a starry-eyed barista. NGC 3895 is a barred spiral galaxy that was first spotted by William Herschel in 1790 and was later observed by the NASA/ESA Hubble Space Telescope. Hubble's orbit high above the Earth's distorting atmosphere allows astronomers to make the very high resolution observations...

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