This Is The Eagle Nebula!Β πŸ¦…πŸ¦…πŸ¦…

This Is The Eagle Nebula!Β πŸ¦…πŸ¦…πŸ¦…

This is the Eagle Nebula!Β πŸ¦…πŸ¦…πŸ¦…

This young cluster of stars and the distinct Pillars of Creation at the center of the nebula are located in the constellation of Serpens. These stars, which were formed in the HII region of this nebula, are very massive: some of them are up to 1 million solar luminosities! ✨✨✨

Taken by me (Michelle Park) using the Slooh Canary Two telescope on May 9th, 2021 at 00:36 UTC.Β 

More Posts from Mystarypi and Others

4 years ago

Hello everyone!Β A few months ago, I released Project DeLightΒ -Β  an initiative against light pollution in our community.

I just made an instagram for this project so please follow us for updates! ✨✨✨

4 years ago
The John Rylands Library
The John Rylands Library
The John Rylands Library

the john rylands library

4 years ago
2020 November 22

2020 November 22

Dark Molecular Cloud Barnard 68 Image Credit: FORS Team, 8.2-meter VLT Antu, ESO

Explanation: Where did all the stars go? What used to be considered a hole in the sky is now known to astronomers as a dark molecular cloud. Here, a high concentration of dust and molecular gas absorb practically all the visible light emitted from background stars. The eerily dark surroundings help make the interiors of molecular clouds some of the coldest and most isolated places in the universe. One of the most notable of these dark absorption nebulae is a cloud toward the constellation Ophiuchus known as Barnard 68, pictured here. That no stars are visible in the center indicates that Barnard 68 is relatively nearby, with measurements placing it about 500 light-years away and half a light-year across. It is not known exactly how molecular clouds like Barnard 68 form, but it is known that these clouds are themselves likely places for new stars to form. In fact, Barnard 68 itself has been found likely to collapse and form a new star system. It is possible to look right through the cloud in infrared light.

∞ Source: apod.nasa.gov/apod/ap201122.html

4 years ago
Join Slooh For A Special Star Party Live On Sunday, June 13th At 1 PM EST! ✨✨✨

Join Slooh for a special Star Party Live on Sunday, June 13th at 1 PM EST! ✨✨✨

The Slooh Ambassadors (which includes me) have been working on this Women are From Venus star party that hopes to encourage women to participate in astronomy! 🎊🎊🎊

Jenny McFarlane will be discussing how she expands astronomy outreach at her planetarium! There will also be other talks made by other Slooh women who are passionate about space. πŸ™ŒπŸ™ŒπŸ™Œ

All you need to do is to make a free account at Slooh.com and then watch the star party on the website! If you are a woman and would like to participate in the Zoom, send an email to paul@slooh.com for the Zoom passcode. Please let me know if you have any questions and I hope you can attend πŸ’–πŸ’–πŸ’–

3 years ago
This Is The Orion Nebula! ✨✨✨

This is the Orion Nebula! ✨✨✨

Recent observations by the Hubble Space Telescope reveal the presence of protoplanetary disks, or proplyds, in the Orion Nebula. Newborn stars form in this beautiful nebula when clumps of hydrogen gas condense and become hot enough for stellar fusion! πŸ’₯πŸ’₯πŸ’₯

Taken by me (Michelle Park) using the Slooh Canary Two telescope on January 20th, 2022 at 3:22 UTC.

4 years ago

One of my favorite nebulae β™₯β™₯β™₯ It looks so beautiful πŸ₯°πŸ₯°πŸ₯°

NGC 6357: Cathedral To Massive Stars Via NASA Https://ift.tt/31D4Lqn

NGC 6357: Cathedral to Massive Stars via NASA https://ift.tt/31D4Lqn

How massive can a normal star be? Estimates made from distance, brightness and standard solar models had given one star in the open cluster Pismis 24 over 200 times the mass of our Sun, making it one of the most massive stars known. This star is the brightest object located just above the gas front in the featured image. Close inspection of images taken with the Hubble Space Telescope, however, have shown that Pismis 24-1 derives its brilliant luminosity not from a single star but from three at least. Component stars would still remain near 100 solar masses, making them among the more massive stars currently on record. Toward the bottom of the image, stars are still forming in the associated emission nebula NGC 6357. Appearing perhaps like a Gothic cathedral, energetic stars near the center appear to be breaking out and illuminating a spectacular cocoon.

(Published August 30, 2020)

4 years ago

One of my best shots of this stunning galaxy! Please follow my astrophotography tumblr (mystarypi-astronomy.tumblr.com) for similar astrophotos like these!

This Is The Silver Coin Galaxy! πŸ’ΈπŸ’ΈπŸ’Έ

This is the Silver Coin Galaxy! πŸ’ΈπŸ’ΈπŸ’Έ

This is one of the brightest and dustiest galaxies known to Earth. With so much dust, star formation is aggressive in this galaxy and thus, it is classified as a starbust galaxy! ✨✨✨

Many scientists think that the star formation may have also been caused by the Silver Coin Galaxy’s collision with a dwarf galaxy billions of years ago! 🌌🌌🌌

Taken by me (Michelle Park) using the Slooh Chile One telescope on October 21st, 2020 at 6:52 UTC.

4 years ago

So beautiful - I absolutely love the night sky! ✨✨✨

Follow my astrophotography tumblr: mystarypi-astronomy.tumblr.com

mystarypi - MystaryPi

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4 years ago
image

Blusighs is typing…

2020λ…„07μ›”07일

Day 2(7)/30 of #30dol

I can’t choose between Noteshelf and OneNote, they’re both great but I’m very indecisive on which I’ll be permanently using. Anyways, today was a slow day so I studied less. Btw some time next week or this week, i’ll be posting my shopee haul ! See you <3Β 

3 years ago
This Is Vega! ✨✨✨

This is Vega! ✨✨✨

This is the brightest star in the summer constellation Lyra and the 5th brightest star in the night sky. Infrared observations have confirmed a circumstellar disk of dust around this star, similar to the Kuiper Belt around the solar system! πŸŒƒπŸŒƒπŸŒƒ

Taken by me (Michelle Park) using the Slooh Canary Two telescope on July 5th, 2021 at 22:26 UTC.Β 

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mystarypi - MystaryPi
MystaryPi

Go to my main ✨: mystarypi-astronomy.tumblr.com

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