Hemisphere:  Northern  ·  Constellation: Ursa Major (UMa)  ·  Contains:  M 101  ·  NGC 5447  ·  NGC 5449  ·  NGC 5450  ·  NGC 5451  ·  NGC 5453  ·  NGC 5455  ·  NGC 5457  ·  NGC 5461  ·  NGC 5462  ·  NGC 5471  ·  Pinwheel galaxy
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The Pinwheel Galaxy (Messier 101 or NGC 5457), 


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The Pinwheel Galaxy (Messier 101 or NGC 5457)

Getting plate-solving status, please wait...
The Pinwheel Galaxy (Messier 101 or NGC 5457), 


Powered byPixInsight

The Pinwheel Galaxy (Messier 101 or NGC 5457)

Acquisition details

May 12, 2019
36×180(1h 48′)
1h 48′
Avg. Moon age:
7.88 days
Avg. Moon phase:
Bortle Dark-Sky Scale:

RA center: 14h03m18s.850

DEC center: +54°2039.61

Pixel scale: 0.551 arcsec/pixel

Orientation: -2.036 degrees

Field radius: 0.336 degrees

More info:Open 

Resolution: 3450x2706

File size: 34.2 MB

Data source: Backyard


Heavily cropped to bring in, I hope to do a lot better than this in the future !

The Pinwheel Galaxy (also known as Messier 101, M101 or NGC 5457) is a face-on spiral galaxy distanced 21 million light-years (six megaparsecs) away from Earth in the constellation Ursa Major. Discovered by Pierre Méchain on March 27, 1781, it was communicated to Charles Messier who verified its position for inclusion in the Messier Catalogue as one of its final entries.

M101 is a large galaxy, with a diameter of 170,000 light-years. By comparison, the Milky Way has a diameter of 258,000[11] light years. It has around a trillion stars, twice the number in the Milky Way.[12] It has a disk mass on the order of 100 billion solar masses, along with a small central bulge of about 3 billion solar masses.

M101 has a high population of H II regions, many of which are very large and bright. H II regions usually accompany the enormous clouds of high density molecular hydrogen gas contracting under their own gravitational force where stars form. H II regions are ionized by large numbers of extremely bright and hot young stars; those in M101 are capable of creating hot superbubbles.[14] In a 1990 study, 1264 H II regions were cataloged in the galaxy.[15] Three are prominent enough to receive New General Catalogue numbers - NGC 5461, NGC 5462, and NGC 5471.[16]

M101 is asymmetrical due to the tidal forces from interactions with its companion galaxies. These gravitational interactions compress interstellar hydrogen gas, which then triggers strong star formation activity in M101's spiral arms that can be detected in ultraviolet images.[17]

In 2001, the x-ray source P98, located in M101, was identified as an ultra-luminous X-ray source - a source more powerful than any single star but less powerful than a whole galaxy - using the Chandra X-ray Observatory. It received the designation M101 ULX-1. In 2005, Hubble and XMM-Newton observations showed the presence of an optical counterpart, strongly indicating that M101 ULX-1 is an x-ray binary.[18] Further observations showed that the system deviated from expected models - the black hole is just 20 to 30 solar masses, and consumes material (including captured stellar wind) at a higher rate than theory suggests.


Sky plot

Sky plot


The Pinwheel Galaxy (Messier 101 or NGC 5457), 



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