d e v o n
No title available
Monterey Bay Aquarium

No title available

if i look back, i am lost
Aqua Utopia|海の底で記憶を紡ぐ
PUT YOUR BEARD IN MY MOUTH
Cosmic Funnies
will byers stan first human second
"I'm Dorothy Gale from Kansas"
No title available
TVSTRANGERTHINGS

Kiana Khansmith
he wasn't even looking at me and he found me
tumblr dot com
taylor price

Origami Around
noise dept.

blake kathryn
2025 on Tumblr: Trends That Defined the Year

seen from T1
seen from United States
seen from Spain
seen from United States
seen from Germany

seen from Japan
seen from United Kingdom
seen from Ukraine

seen from Singapore

seen from Switzerland

seen from Switzerland
seen from United States
seen from Chile
seen from Portugal

seen from United States
seen from Argentina

seen from Nepal
seen from United States
seen from Brazil
seen from United States
@jonx-rodrx
Moody and misty
Bavaria. Germany
Tú estás en sus dms y yo ya aprendí a dejar ir lo que no es bueno para mí.
NGC 247
The spiral galaxy NGC 247 may not look particularly spiral, but it's a 75,000 light year across galaxy not too dissimilar to our Milky Way, the difference being from Earth, it appears near side-on, hiding the arms and features we associate with a spiral.
One interesting aside is the Burbidge's Chain, 4 galaxies lined up, and with the left two appearing to show some kind of star connection between them.
NGC 247 is 11 million light years from Earth in the constellation of Cetus, while the 4 in the chain, are much further back, around 300 million light years from Earth.
NGC 5668
90 million light years from Earth in the constellation of Virgo lies this barred spiral galaxy, and it has a fair amount in common with our Milky Way, similar in size and mass, but it's blue colour gives away a few differences too, as this galaxy is producing stars 60% more than our own galaxy.
Hubble recently took this beautiful image, to help astronomers understand why.
It's thought the process is driven by two factors, firstly the oval shape of the central bar, seems to produce conditions which feed dust and gas that then in significant quantities form stars.
Secondly there's also a flow of dust and gas outwards towards the halo, leaving the disk and moving towards this faint structure, you can see significant star formation on the outer edges, like diamonds.
The movement of dust and gas causes a bow shockwave which in turn collects more dust and gas that was sitting around, making areas of very dense material that can form stars.
When it comes to galaxies, never judge a book by a glance at the cover, look closely and you'll see even a spiral can hide many unique features.
Solar eclipse
On The Road, Again (2022) Get back up on your feet, yea? Twitter | Ko-Fi | Patreon
eleuiggi by florian hetz
storm brew
lake kaweah, california
si soy