NGC 2158

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Open star cluster
NGC 2158
SDSS recording, angle of view 13.5 '× 13.5'
SDSS recording, angle of view 13.5 '× 13.5'
AladinLite
Constellation Twins
Position
equinox : J2000.0
Right ascension 06 h 07 m 25.6 s
declination + 24 ° 05 ′ 46 ″
Appearance

classification II3r
Brightness  (visual) 8.6 likes
Brightness  (B-band) 9.49 likes
Angular expansion 5 '
Number of stars > 10,000 stars
Brightest star +12 to +13 mag
Variable stars 97
Redness ( excess color  E (BV)) 0.360
Physical data

distance  approx. 16200 ly
(4980 pc )
Age > 1 billion years
history
Discovered by Wilhelm Herschel
Discovery time November 16, 1784
Catalog names
 NGC  2158 • C 0604 + 241 • OCl 468 •  Mel  40 •  Cr  81 • Lund 205 •  GC  1351 •  H  VI 17 •  h  375 • Raab 30

NGC 2158 is an open star cluster in the constellation Gemini . It is only about 15 'southwest of the edge of the much brighter M35 cluster . The star cluster, discovered by Wilhelm Herschel on November 16, 1784 , has an apparent diameter of only 5 'and a brightness of 8.6 mag. The stars of the more than 1 billion year old star cluster are highly concentrated, similar to a globular cluster . That is why he used to be thought of as such; due to its age, however, the identification as an open star cluster is clear.

If you have NGC 2158 together with M35 in the telescope's field of view, the contrast in size and star density is particularly clear. NGC 2158 is five times farther away, but has at least 10 times more stars and is much older.

Web links

Individual evidence

  1. NASA / IPAC EXTRAGALACTIC DATABASE
  2. a b SEDS : NGC 2158
  3. SIMBAD database
  4. a b GoBlack: NGC 2158 open star cluster in the constellation Gemini
  5. Papers: Planets in Stellar Clusters Extensive Search. IV. A detection of a possible transiting planet candidate in the open cluster NGC 2158 ( Memento from October 7, 2006 in the Internet Archive )
  6. webda.physics.muni.cz: WEBDA page for open cluster NGC 2158 , accessed on May 3, 2019
  7. AL Tadross: A catalog of 120 NGC open star cluster . In: Journal of the Korean Astronomical Society , 44, 2011, pp. 1-11. doi: 10.5303 / JKAS.2011.44.1.1 .
  8. Seligman