Open Cluster NGC 2129

NGC 2129
NGC 2129: Section of DSS2. Here could be your picture. [147]

History

This open cluster was discovered on 6 February 1782 by German-British astronomer William Herschel, although he did not recognize it then as such. He was conducting his third star review using his 6.2" reflector and catalogued it as the multiple star IV. 48 for which he noted: «Quintuple. In the form of a cross. About 2/3 degree north preceding H Geminorum, in a line parallel to the 65th Orionis and ζ Tauri; the middle of three. The two nearest or preceding of the five extremely unequal. Distance 20'' 57'''. Position 7° 27' south preceding. The last of the three, in the short bar of the cross, has an excessively obscure star near it of the third class. Five more in view, differently dispersed about the quintuple.» [734]

On 16 Nov 1784 Herschel rediscovered this cluster while he was sweeping the sky with his 18.7-inch speculum reflector of 20 feet focal length in Datchet, near to Windsor Castle. He listed the cluster as VIII 26 and noted: «A Cluster of stars of various magnitudes, not very rich, 6 or 7' diameter.» [463]

Continuing his father's work, John Herschel observed the cluster on 24 February 1827 (sweep 59), listed it as h 372 and wrote: «About 40 or 50 stars. The brightest 8 mag taken. The rest are 10...15 mag.» [466]

Physical Properties

NGC 2129 is a young, compact star cluster with a radius of 2.0–2.5 arcminutes, corresponding to about 1.0–1.3 parsecs at its estimated distance. Located roughly 2200 parsecs from the Sun in the direction of the Galactic anticentre, it lies within the Local Spiral Arm. The cluster contains 37 probable member stars with spectral types earlier than A5. It exhibits a mean reddening of E(B − V) = 0.82 ± 0.08, along with significant differential reddening across the region. The cluster's estimated age is around 10 million years. [738]

Revised+Historic NGC/IC Version 22/9, © 2022 Dr. Wolfgang Steinicke [277]
DesignationNGC 2129
TypeOCL (III3p)
Right Ascension (J2000.0)06h 01m 06.5s
Declination (J2000.0)+23° 19' 04"
Diameter6 arcmin
Visual magnitude6.7 mag
Metric Distance1.515 kpc
Dreyer DescriptionCl, pL, 40 or 50 st 8…15
Identification, RemarksWH VIII 26; h 372; GC 1325; OCL 467

Finder Chart

The open cluster cluster NGC 2129 can be found in the constellation Gemini. On 23 December it in opposition with the Sun and is therefore highest in the sky at local midnight.

Gemini: Open Cluster NGC 2129
Finder Chart Open Cluster NGC 2129
01:52
09:08 | 66.5°
16:24
Charts created using SkySafari 6 Pro and STScI Digitized Sky Survey. Limiting magnitudes: Constellation chart ~6.5 mag, DSS2 close-ups ~20 mag. Times are shown for timezone UTC, Latitude 46.7996°, Longitude 8.23225°, Horizon height 5°, Date 2025-07-27. [149, 160]

Objects Within a Radius of 10°

References

  • [147] Aladin Sky Atlas, Centre de Données astronomiques de Strasbourg (CDS); aladin.unistra.fr
  • [149] SkySafari 6 Pro, Simulation Curriculum; skysafariastronomy.com
  • [160] The STScI Digitized Sky Survey; archive.stsci.edu/cgi-bin/dss_form
  • [277] Historische Deep-Sky Kataloge; Dr. Wolfgang Steinicke; klima-luft.de/steinicke; 2021-02-17
  • [463] Catalogue of one thousand new nebulae and clusters of stars; William Herschel; Philosophical Transactions of the Royal Society of London, 1 January 1786; DOI:10.1098/rstl.1786.0027
  • [466] Observations of nebulæ and clusters of stars, made at Slough, with a twenty-feet reflector, between the years 1825 and 1833; John Frederick William Herschel; Philosophical Transactions of the Royal Society of London, 1 January 1833, Pages: 359-505; DOI:10.1098/rstl.1833.0021
  • [734] VI. Catalogue of double stars; William Herschel; Philosophical Transactions of the Royal Society of London, Volume 75, Dec 1785; DOI:10.1098/rstl.1785.0006
  • [738] The young open cluster NGC 2129; Giovanni Carraro, Brian Chaboyer, James Perencevich; Monthly Notices of the Royal Astronomical Society, Volume 365, Issue 3, January 2006, Pages 867–873; DOI:10.1111/j.1365-2966.2005.09762.x