Hemisphere:  Northern  ·  Constellation: Auriga (Aur)  ·  Contains:  M 38  ·  NGC 1912
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M38 above the full moon, 



    
        

            Rob Johnson
M38 above the full moon
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M38 above the full moon

Technical card

Imaging telescopes or lenses: Telescope Service 12" f5

Mounts: EQ8

Guiding telescopes or lenses: Telescope Service 12" f5

Guiding cameras: QHYCCD Qhy5L II

Software: Pleiades Astrophoto PixInsight 1.8 PixInsight

Filters: Optolong 36mm LRGB


Dates:Feb. 26, 2021

Frames: 27x120" bin 2x2

Integration: 0.9 hours

Avg. Moon age: 13.85 days

Avg. Moon phase: 99.05%

Bortle Dark-Sky Scale: 8.00

Mean FWHM: 3.80


Basic astrometry details

Astrometry.net job: 4259041

RA center: 5h 28' 41"

DEC center: +35° 51' 14"

Pixel scale: 1.465 arcsec/pixel

Orientation: 358.272 degrees

Field radius: 0.428 degrees


Resolution: 1681x1268

Locations: Thingwall observatory, Liverpool, United Kingdom

Data source: Backyard

Description

Well a high pressure system over the UK means....a full moon! Neverthless clusters are an easy target even with added illumination. I have always liked the three Messier clusters in Auriga which are beautiful to browse from a dark sky site.
This image was a little under an hour in RGB.

From Wikipedia: Messier 38 or M38, also known as NGC 1912 or Starfish Cluster,[4] is an open cluster of stars in the constellation of Auriga. It was discovered by Giovanni Batista Hodierna before 1654 and independently found by Le Gentil in 1749. Open cluster M36 and M37, also discovered by Hodierna, are often grouped together with M38.[5] Distance is about 1.066 kpc (3,480 ly) away from Earth.[2] The open cluster NGC 1907 lies nearby on the sky, but the two are most likely just experiencing a fly-by, having originated in different parts of the galaxy.[1]

The cluster's brightest stars form a pattern resembling the Greek letter Pi or, according to Webb, an "oblique cross". Walter Scott Houston described its appearance as follows:[6]

"Photographs usually show a departure from circularity, a feature quite evident to visual observers. Older reports almost always mention a cross shape, which seems more pronounced with small instruments. A view with a 24-inch reflector on a fine Arizona night showed the cluster as irregular, and the host of stars made fruitless any effort to find a geometrical figure."

At its distance of 1066 pc., its angular diameter of about 20 arc minutes corresponds to about 4.0 parsecs (13 light years), similar to that of its more distant neighbor M37. It is of intermediate age at about 290 million years.[2] From the population of about 100 stars,[7] this open cluster features a prominent yellow giant with the apparent magnitude +7.9 and spectral type G0 as its brightest member. This corresponds to an absolute magnitude of -1.5, or a luminosity of 900 Suns. For comparison, the Sun would appear as a faint magnitude +15.3 star from the distance of M38.

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