safelymythicalwonder
safelymythicalwonder
Untitled
20 posts
Don't wanna be here? Send us removal request.
safelymythicalwonder · 9 days ago
Text
Tumblr media Tumblr media
12K notes · View notes
safelymythicalwonder · 9 days ago
Text
Tumblr media Tumblr media Tumblr media Tumblr media
(1) Gustavo Tavares (2) Daniel Mišúr (3) David Kopacz (4) Robert Gruszecki
2K notes · View notes
safelymythicalwonder · 9 days ago
Text
Tumblr media Tumblr media Tumblr media Tumblr media
Robert Gruszecki
6K notes · View notes
safelymythicalwonder · 20 days ago
Text
the magnificence of the stars 🌟 ✨✨
17K notes · View notes
safelymythicalwonder · 20 days ago
Text
Tumblr media
8 notes · View notes
safelymythicalwonder · 21 days ago
Text
Tumblr media
22 notes · View notes
safelymythicalwonder · 25 days ago
Text
Tumblr media
4K notes · View notes
safelymythicalwonder · 25 days ago
Text
Tumblr media
M27 /NGC 6853 The Dumbbell Nebula
296 notes · View notes
safelymythicalwonder · 25 days ago
Text
Tumblr media
23 notes · View notes
safelymythicalwonder · 25 days ago
Text
Tumblr media
Muir Woods, CA - Author: erikfournier
228 notes · View notes
safelymythicalwonder · 25 days ago
Note
Send me a message now
Hi sir...what do you want to know? I am 18, fit slim, smooth, horny a wild twink. I am from South London and I have a boyfriend frm college. We do parties together...and entertain guests!
0 notes
safelymythicalwonder · 25 days ago
Note
Have you been owned by a master
Not owned by one, but been used by many!
0 notes
safelymythicalwonder · 26 days ago
Text
Tumblr media
Taylor Anderson
21 notes · View notes
safelymythicalwonder · 29 days ago
Text
Tumblr media
10 billion light-years away...
Giant Star Seen 150 Days Before it Exploded as a Supernova !
In April of 2023, a massive star exploded in NGC 4388, a spiral galaxy about 57 million light-years away. The Zwicky Transient Facility (ZTF) spotted it, and the supernova is called SN 2023 fyg. SN 2023fyq is a rare type of supernova called a Type Ibn.
They show a lack of hydrogen lines and narrow He I emission lines in their spectra. Astronomers think that these characteristics come from the SN interacting with hydrogen-poor, helium-rich circumstellar material (CSM.)
Astronomers only know of a few of these types of SN, so their progenitors are poorly understood. Prior to its explosion, the ZTF also spotted the precursor activity, providing a window into these mysterious progenitors.
33 notes · View notes
safelymythicalwonder · 29 days ago
Text
Tumblr media
This view is therapeutic. - Author: LavenderStaticy
6K notes · View notes
safelymythicalwonder · 29 days ago
Text
Play time!
thesilentwanderers
7K notes · View notes
safelymythicalwonder · 29 days ago
Text
Tumblr media Tumblr media
by kevin.ksp5
12K notes · View notes