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NGC 2302

From Wikipedia, the free encyclopedia
(Redirected from NGC 2299)
NGC 2302
NGC 2302 imaged by Pan-STARRS
Observation data
Right ascension06h 51m 53.67s[1]
Declination−07° 04′ 54.8″[1]
Distance3.78 ± 0.26 kly (1.16 ± 0.08 kpc)[2]
Apparent dimensions (V)30′[2]
Physical characteristics
Mass333±48[2] M☉
Radius17 ly (5.1 pc)[2]
Estimated age80 ± 20 Myr[2]
Associations
ConstellationMonoceros
See also: Open cluster, List of open clusters

NGC 2302 (also called NGC 2299) is an open cluster[3] in the constellation Monoceros.[4] It was discovered on March 4, 1785, by William Herschel (and later listed as NGC 2302)[5][4] and separately on January 19, 1828 by John Herschel (and later listed as NGC 2299).[5][6]

A low-mass open cluster, NGC 2302 has a stellar mass of about 333 times that of the Sun. NGC 2302 is about 80 million years old. Based on Gaia parallaxes, NGC 2302 is about 3,800 light-years (1,160 parsecs) away from the Sun. With an apparent radius of 15′, this corresponds to a physical radius of about 17 light-years (5.1 parsecs).[2]

References

[edit]
  1. 1 2 "NASA/IPAC Extragalactic Database (NED) results for object NGC 2302". NASA/IPAC. Retrieved 2026-04-10.
  2. 1 2 3 4 5 6 Lee, Yuna; Hong, Jongsuk; Lim, Beomdu (2026). "Kinematics and Dynamics of the Open Cluster NGC 2302". Journal of the Korean Astronomical Society. 59 (2): 367–377. arXiv:2608.18550. Bibcode:2026JKAS...59..367L. doi:10.5303/JKAS.2026.59.2.367.
  3. ↑ "NGC 2302". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2026-04-10.
  4. 1 2 "New General Catalog Objects: NGC 2300 - 2349". cseligman.com. Retrieved 2026-04-10.
  5. 1 2 "New General Catalog Objects: NGC 2250 - 2299". cseligman.com. Retrieved 2026-04-10.
  6. ↑ Costa, Edgardo; Moitinho, André; Radiszc, Matías; Muñoz, Ricardo R.; Carraro, Giovanni; Vázquez, Ruben A.; Servajean, Elise (August 2015). "Insights into the properties of the Local (Orion) spiral arm. NGC 2302: First results and description of the program". Astronomy & Astrophysics. 580: A4. arXiv:1505.01872. doi:10.1051/0004-6361/201525784. ISSN 0004-6361.