NGC 3000 explained

NGC 3000
Epoch:J2000
Constellation Name:Ursa Major
Dec:+44° 07’ 49”
Ra:09h 48m 51s
Dist Ly:168 Mly (51.66 Mpc)
Appmag V:10.88
Type:SB(r)bc
Notes:N/A
Names:PGC 5067534
Appmag B:11

NGC 3000 is a double star located in the constellation Ursa Major.[1] It was first discovered and observed by Bindon Stoney an assistant to William Parsons, on January 25, 1851,[2] and was initially catalogued as a nebula-like object. Since its discovery, NGC 3000 has been observed and studied using various telescopes.

Discovery

Bindon Stoney first described NGC 3000 as a "very faint, small, irregularly round, mottled but not resolved" galaxy. However, its recorded position, precessed to RA 09 49 02.6, Dec +44 08 46, shows no object at that location. Analysis reveals Stoney's recorded positions for objects in this region consistently have a systematic error of approximately 2 arcminutes to the east-northeast. Applying this correction places the coordinates nearly precisely on a pair of stars now identified as NGC 3000.[3]

Notes and References

  1. Web site: Ford . Dominic . The New General Catalogue (NGC) in Ursa Major . 2024-03-20 . In-The-Sky.org . en.
  2. Web site: NGC 3000 . 2024-03-20 . spider.seds.org.
  3. Web site: New General Catalog Objects: NGC 3000 - 3049 . 2024-03-20 . cseligman.com.