Palomar 1

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Palomar 1
Palomar 1 Hubble WikiSky.jpg
Palomar 1 by Hubble Space Telescope; 3.3′ view
Credit: NASA/STScI/WikiSky
Observation data (J2000 epoch)
Class XII
Constellation Cepheus
Right ascension 03h 33m 20.04s[1]
Declination +79° 34′ 51.8″[1]
Distance 36.5 ± 4.2 kly (11,200 ± 1,300 pc)[2]
Apparent magnitude (V) +13.18
Apparent dimensions (V) 2′.8
Physical characteristics
Radius 15 ly[3]
Estimated age 6.3 to 8 Gyr[2]
Notable features -
Other designations LEDA 13165[4]
See also: Globular cluster, List of globular clusters

Palomar 1 is a globular cluster in the constellation Cepheus in the halo or Outer Arm(?) of the Milky Way galaxy. First discovered by George O. Abell in 1954 on the Palomar Survey Sky plates,[5] it was catalogued as a globular cluster. At 6.3 to 8 Gyr, it is a very young cluster when compared to the other globular clusters in the Milky Way.[2] It is a relatively metal-rich globular with [Fe/H] = -0.60.[6] It is likely that Palomar 1 has a similar evolutionary history to the Sagittarius dwarf companion globular Terzan 7, that is, it may have once been associated with a dwarf spheroidal galaxy that was later destroyed by tidal forces.[6]

References

  1. 1.0 1.1 Lua error in package.lua at line 80: module 'strict' not found.
  2. 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
  3. distance × sin( diameter_angle / 2 ) = 15 ly. radius
  4. Lua error in package.lua at line 80: module 'strict' not found.
  5. Lua error in package.lua at line 80: module 'strict' not found.
  6. 6.0 6.1 Lua error in package.lua at line 80: module 'strict' not found.

External links

Coordinates: Sky map 03h 33m 19.3s, +79° 34′ 55″


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