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NGC 358

From Wikipedia, the free encyclopedia
Open cluster in the constellation Cassiopeia
NGC 358
NGC 358 withPanSTARRS
Observation data (J2000.0epoch)
Right ascension01h 05m 11.00s[1]
Declination+62° 01′ 18.0″[1]
Distance1700 ± 300
Apparent dimensions (V)2.5[2]
Physical characteristics
Associations
ConstellationCassiopeia
See also:Open cluster,List of open clusters

NGC 358 is anasterism of four stars in the constellation ofCassiopeia. Two of the members were found to have a similar distance of roughly 1700 light years withHipparcos data, although the other two did not have well-constrained distances, so its exact nature was uncertain.

Gaia DR3 data shows that the two members TYC 4021-519-1 and TYC 4021-575-1 are not associated due to their very differentproper motion andradial velocity. The distance remains remarkable similar for both stars from the Gaiaparallax. The other two stars have larger distances.[3]

The asterism was discovered on February 4, 1865, by the German-Danish astronomerHeinrich Louis d'Arrest.[4]

Individual Objects

[edit]
ComponentRight AscensionDeclinationDistance (parsec)BrightnessReference
TYC 4021-519-101h 05m 03.5s+62° 01′ 41.4″537 ± 511.2
TYC 4021-575-1
CMC 600551
01h 05m 15.4s+62° 01′ 37.1″544 ± 411.8Gaia DR3
TYC 4021-649-101h 05m 05.7s+62° 00′ 54.5″947 ± 1411.6Gaia DR3
USNO-A2.0 1500-0112097401h 05m 19s+62° 00′ 57″3238+144
−131
12.5Gaia DR3

USNO-A2.0

References

[edit]
  1. ^ab"NGC 358".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved14 December 2017.
  2. ^Students for the Exploration and Development of SpaceArchived 2007-10-20 at theWayback Machine
  3. ^abGaia Collaboration (2022-05-01)."VizieR Online Data Catalog: Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)".VizieR Online Data Catalog: I/355.Bibcode:2022yCat.1355....0G.
  4. ^Seligman, Courtney."NGC 358".Celestial Atlas. Retrieved7 December 2018.

External links

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