Little Ghost Nebula
via APOD/NASA; credit: Hubble Heritage Team, NASA
Sweet Seals For You, Always

oozey mess
Not today Justin
Keni

#extradirty
The Stonewall Inn

Jar Jar Binks Fan Club
𓃗
$LAYYYTER
Noah Kahan

No title available

PR's Tumblrdome
cherry valley forever

shark vs the universe
almost home
noise dept.

Kiana Khansmith

No title available

roma★
Cosmic Funnies
seen from Saudi Arabia

seen from United States
seen from Bulgaria
seen from Pakistan
seen from Brazil

seen from United States
seen from Russia

seen from United Kingdom

seen from Italy
seen from Uzbekistan
seen from Türkiye
seen from United Kingdom
seen from Canada
seen from Russia

seen from Netherlands
seen from United States
seen from United States

seen from United States

seen from Norway
seen from Dominican Republic
@iliveinaspiralgalaxy
Little Ghost Nebula
via APOD/NASA; credit: Hubble Heritage Team, NASA
Veil HaOiiirgb by Risteard O'Suibhne on Flickr.
Propeller Nebula (Simeis 57) in HSTrgb by Jose Carballada Via Flickr: www.astrobin.com/368569 The peculiar nebula Simeis 57. Simeis 57 (also known as HS 191 and C 191) is a high surface-brightness nebula in the constellation Cygnus. The distance nor the source of excitation of Simeis 57 are known.
Among Sagittarius and Scorpius by Lamberto Sassoli
Lunar Eclipse 2018 by Martin Heigan
The Lonely Neutron Star in Supernova Remnant E0102-72.3 by NASA’s Marshall Space Flight Center on Flickr.
Multispectral Sun
Credit: NASA/SDO/GSFC
Interstellar Dome by Muhammad Elarbi
M31, M32 and NGC206 by Cristiano Secci
SH2-157 Lobster Claw Nebula by eBear Foto
@ T h e T r a v e l l e r s ( Redit ) by VegaStarCLiardPhotography Via Flickr: ©VegaStarCLiardP h o t o g r a p h y vegastarcarpentierphotography.wordpress.com
“Most galaxies don’t have any rings – why does this galaxy have two? To begin, the bright band near NGC 1512’s center is a nuclear ring, a ring that surrounds the galaxy center and glows brightly with recently formed stars. Most stars and accompanying gas and dust, however, orbit the galactic center in a ring much further out – here seen near the image edge. This ring is called, counter-intuitively, the inner ring. If you look closely, you will see this the inner ring connects ends of a diffuse central bar that runs horizontally across the galaxy. These ring structures are thought to be caused by NGC 1512’s own asymmetries in a drawn-out process called secular evolution. The gravity of these galaxy asymmetries, including the bar of stars, cause gas and dust to fall from the inner ring to the nuclear ring, enhancing this ring’s rate of star formation. Some spiral galaxies also have a third ring – an outer ring that circles the galaxy even further out.”
via APOD/NASA; Credit: NASA, ESA, Hubble Space Telescope
A Surprisingly Bright Superbubble (NASA, Chandra, 08/30/12) by NASA's Marshall Space Flight Center
This photo of water geysers spouting from Saturn’s moon Enceladus was taken by NASA’s Cassini orbiter in October 2007
Credit: Cassini Imaging Team, SSI, JPL, ESA, NASA
Rho Ophiuchi
by: Alex Obrad
The Horsehead Nebula Artprize 2013 entry at GRAM by Terry Hancock
Small Magellanic Cloud with FSQ-106ED and F3 Reducer 0.6x August 2018 Dark Version by hirocun on Flickr.