☆ SPACE / KEVIN / COSMOS ☆
HE / IT ☆ 22 ☆ SIDEBLOG
MAIN: JOKERSJR

oozey mess

shark vs the universe

blake kathryn

JBB: An Artblog!
🪼
$LAYYYTER
ojovivo
Show & Tell
todays bird

Product Placement
Peter Solarz
cherry valley forever

#extradirty

@theartofmadeline
Cosimo Galluzzi
we're not kids anymore.
Lint Roller? I Barely Know Her

pixel skylines

Janaina Medeiros

seen from Bulgaria
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seen from United States
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seen from Bolivia
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@spacecourse
☆ SPACE / KEVIN / COSMOS ☆
HE / IT ☆ 22 ☆ SIDEBLOG
MAIN: JOKERSJR

Anya is live and ready to show you everything. Watch her strip, dance, and perform exclusive shows just for you. Interact in real-time and make your fantasies come true.
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With NASA announcing their streaming service NASA+ and also announcing it’s going to be free and also ad free, I’d just like to appreciate the lengths they go to make scientific knowledge and exploration as available as they possibly can.
There's more info at this link. Gosh I'm excited about this.
NASA is elevating its digital platforms for the benefit of all by revamping its flagship and science websites, adding its first on-demand st
10. 9. 8. 7. 6. 5. 4. 3. 2. 1.
AAAND WE HAVE LIFTOFF!
HAPPY MOON LANDING DAY!!!
Rho Ophiuchi cloud cluster
~Happy anniversary to the James Webb Space Telescope~

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The Tarantula Nebula, also known as 30 Doradus, is more than a thousand light-years in diameter, a giant star forming region within nearby satellite galaxy the Large Magellanic Cloud. About 160 thousand light-years away, it's the largest, most violent star forming region known in the whole Local Group of galaxies. The cosmic arachnid is near the center of this spectacular image taken during the flight of SuperBIT (Super Pressure Balloon Imaging Telescope), NASA's balloon-borne 0.5 meter telescope now floating near the edge of space.
Image Credit: SuperBIT, NASA
Alvin Wu’s Milky Way Ring
Youthful NGC 362 by europeanspaceagency
In the Centre of the Virgo Cluster
Credits: Jean-Charles Cuillandre, Hawaiian Starlight, CFHT
Behold Saturn in a new light! This is an ultraviolet image of glowing hydrogen in Saturn’s atmosphere. It is being heated by material falling from the planet’s rings.
The rings appear much darker than the planet’s body because they reflect much less ultraviolet sunlight. An extended latitudinal band is 30% brighter in ultraviolet light than the surrounding regions.
Credit: NASA, ESA, and Lotfi Ben-Jaffel (Institute of Astrophysics/University of Paris and University of Arizona).

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Saturn - photos (polarised: false colour) respectively taken on the 19 of August 2012, and the 11 of March 2006. NASA.
Hubble Pinpoints Farthest Protocluster of Galaxies Ever Seen by NASA Goddard Photo and Video
Young star offers a glimpse of the Sun’s past by europeanspaceagency
M24, Star Cloud Of Sagittarius
Sakura to Supernova
This rare sight is a super-bright, massive Wolf-Rayet star. Calling forth the ephemeral nature of cherry blossoms, the Wolf-Rayet phase is a fleeting stage that only some stars go through soon before they explode.
The star, WR 124, is 15,000 light-years away in the constellation Sagittarius. It is 30 times the mass of the Sun and has shed 10 Suns worth of material – so far. As the ejected gas moves away from the star and cools, cosmic dust forms and glows in the infrared light detectable by NASA's James Webb Space Telescope.
The origin of cosmic dust that can survive a supernova blast is of great interest to astronomers for multiple reasons. Dust shelters forming stars, gathers together to help form planets, and serves as a platform for molecules to form and clump together, including the building blocks of life on Earth.
Stars like WR 124 also help astronomers understand the early history of the universe. Similar dying stars first seeded the young universe with heavy elements forged in their cores – elements that are now common in the current era, including on Earth.
The James Webb Space Telescope opens up new possibilities for studying details in cosmic dust, which is best observed in infrared wavelengths of light. Webb’s Near-Infrared Camera balances the brightness of WR 124’s stellar core and the knotty details in the fainter surrounding gas. The telescope’s Mid-Infrared Instrument reveals the clumpy structure of the gas and dust nebula of the ejected material now surrounding the star.
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Gravity s Grin : Albert Einstein’s general theory of relativity, published over 100 years ago, predicted the phenomenon of gravitational lensing. And that’s what gives these distant galaxies such a whimsical appearance, seen through the looking glass of X-ray and optical image data from the Chandra and Hubble space telescopes. Nicknamed the Cheshire Cat galaxy group, the group’s two large elliptical galaxies are suggestively framed by arcs. The arcs are optical images of distant background galaxies lensed by the foreground group’s total distribution of gravitational mass. Of course, that gravitational mass is dominated by dark matter. The two large elliptical “eye” galaxies represent the brightest members of their own galaxy groups which are merging. Their relative collisional speed of nearly 1,350 kilometers/second heats gas to millions of degrees producing the X-ray glow shown in purple hues. Curiouser about galaxy group mergers? The Cheshire Cat group grins in the constellation Ursa Major, some 4.6 billion light-years away. via NASA
A Deep Sky Behind an Eclipsed Moon : The plan was to capture a picturesque part of the sky that was hosting an unusual guest. The result included a bonus — an additional and unexpected guest. The beautiful background features part of the central band of our Milky Way galaxy on the far left, and the colorful clouds of Rho Ophiuchi in the image center. The unusual guest, a dimmed and reddened Moon on the right, was expected because the image was taken during last week’s total lunar eclipse. The timing had to be right because the Moon — both before and after eclipse — would be so bright it would overwhelm the background. The unexpected guest was the bright meteor across the image center. The fleeting meteor streak was captured on only one of the 10 consecutively-captured deep-field images from La Palma in the Spanish Canary Islands, while the eclipsed Moon image was taken immediately afterwards with the same camera and from the same location. The next total lunar eclipse — also quite expected — will occur in early November. via NASA