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| Name / Constellation | M 38 |
Other: NGC 1912, Cr 67, Mel 36, OCL 433, Lund 181, GC 1119 | Aur |
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| Coordinates | AR: 05h 28m 42,1s - Dec: +35° 51′ 18″ | |||
| Optics | Takahashi FSQ 106N APO Fluorite F5 - 60/220 guiding refractor | |||
| Camera-Mount | SBIG STF8300M - Orion StarShot Guider - 10Micron GM2000 QCI Mount | |||
| Filters | Baader RGB | |||
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| Location / Date | Promiod (Valle D'Aosta-Italy) "TLP" Remote Observatory - 05 apr 2018 | |||
| Seeing | About 3.8 " @ 2.1 arcosec/pixel unbinned | |||
| Note | ||||
| Acquisition | MaxIm DL - CCD Autopilot 5 | |||
| Processing | Adobe Photoshop CS5 -  |
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| Comment | Messier 38 (also known as M38 or NGC 1912) is an open cluster 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, and often grouped together with M38. Distance is about 1.066 kpc (3,480 ly) away from Earth. The cluster's brightest stars form a pattern resembling the Greek letter Pi or, according to Webb, an "oblique cross." 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. From the population of about 100 stars, 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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