Jump to content

NGC 1783: Difference between revisions

From Wikipedia, the free encyclopedia
Content deleted Content added
m Minor punctuation
m Added Dorado (constellation) and Astronomical objects discovered in 1835 category
Line 37: Line 37:
| age =
| age =
| notes =
| notes =
| names =
| names = ESO 85-SC29
}}
}}


'''NGC 1783''' is a globular cluster in the [[Large Magellanic Cloud]], a satellite dwarf galaxy of the [[Milky Way]]. It is one of the brightest globular clusters in the LMC as viewed from Earth. It was discovered in 1835 by [[John Herschel]]. The compiler of the [[New General Catalogue]], [[John Louis Emil Dreyer]], described this cluster as "considerably bright, large, round, very gradually pretty much brighter middle, mottled but not resolved."<ref name="cseligman"></ref>
'''NGC 1783''' (also known as '''ESO 85-SC29''') is a [[globular cluster]] within the [[Dorado]] constellation and part of the [[Large Magellanic Cloud]], a satellite dwarf galaxy of the [[Milky Way]]. It is one of the brightest globular clusters in the LMC as viewed from Earth. It was discovered in 1835 by [[John Herschel]]. The compiler of the [[New General Catalogue]], [[John Louis Emil Dreyer]], described this cluster as "considerably bright, large, round, very gradually pretty much brighter middle, mottled but not resolved."<ref name="cseligman"></ref>


==References==
==References==
Line 47: Line 47:
[[Category:Globular clusters]]
[[Category:Globular clusters]]
[[Category:NGC objects|1783]]
[[Category:NGC objects|1783]]
[[Category:Dorado (constellation)]]
[[Category:Astronomical objects discovered in 1835]]

Revision as of 18:43, 23 October 2017

NGC 1783
Hubble Space Telescope image of NGC 1783 [1]
Observation data (J2000 epoch)
ConstellationDorado [2]
Right ascension04h 59m 08.6s [3]
Declination−65° 59′ 15.8″ [3]
Distance160 Kly [4] (49 Kpc [4])
Apparent magnitude (V)10.93 [3]
Apparent dimensions (V)5.3' x 4.7' [3]
Physical characteristics
Other designationsESO 85-SC29
See also: Globular cluster, List of globular clusters

NGC 1783 (also known as ESO 85-SC29) is a globular cluster within the Dorado constellation and part of the Large Magellanic Cloud, a satellite dwarf galaxy of the Milky Way. It is one of the brightest globular clusters in the LMC as viewed from Earth. It was discovered in 1835 by John Herschel. The compiler of the New General Catalogue, John Louis Emil Dreyer, described this cluster as "considerably bright, large, round, very gradually pretty much brighter middle, mottled but not resolved."[2]

References

  1. ^ "A youthful cluster". ESA/Hubble Picture of the Week. Retrieved 24 August 2015.
  2. ^ a b "New General Catalogue Objects: NGC 1750 - 1799". Retrieved 2015-09-20.
  3. ^ a b c d "SIMBAD Astronomical Database". Results for NGC 1783. Retrieved 2015-09-20.
  4. ^ a b "NASA/IPAC Extragalactic Database". Results for NGC 1783. Retrieved 2015-09-20.