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NGC 527

Coordinates:Sky map01h 23m 58.0s, -35° 06′ 55″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Sculptor
NGC 527
NGC 527
NGC 527 as seen byDECam
Observation data (J2000[1]epoch)
ConstellationSculptor[2]
Right ascension01h 23m 58.0s[3]
Declination−35° 06′ 55″[3]
Redshift0.019243 ± 0.000057[1]
Heliocentric radial velocity(5713 ± 17) km/s[1]
Distance259Mly[4]
Apparent magnitude (V)13.2[2]
Apparent magnitude (B)14.1[2]
Characteristics
TypeSB0-a[2]
Apparent size (V)1.6' × 0.3'[2]
Other designations
PGC 5128,PGC 5141,GC 310,MGC -06-04-021,2MASS J01235812-3506545,h 2409[1][5]

NGC 527, also occasionally referred to asPGC 5128 orPGC 5141, is alenticular galaxy located approximately 259 million light-years from theSolar System[4] in the constellationSculptor.[2] It was discovered on 1 September 1834 byastronomerJohn Herschel.[5]

Observation history

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Herschel discovered the object along withNGC 526.[6] The object was later catalogued byJohn Louis Emil Dreyer in the New General Catalogue, where the galaxy was described as "faint, small, a little extended, brighter middle, the following (eastern) of 2" with the other one being NGC 526.[5]

Description

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The galaxy has anapparent visual magnitude of 13.2 and can be classified as type SB0-a using theHubble Sequence.[2] The object's distance of roughly 260 million light-years from the Solar System can be estimated using itsredshift andHubble's law.[4]

Companion galaxy PGC 5142

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NGC 527 has a much dimmer magnitude 14 companion galaxy (PGC 5142). Although this galaxy is not an NGC object, it is sometimes referred to as NGC 527B. The galaxy has an apparent size of 1.6' × 0.3' and a recessional velocity of approximately 5880 km/s.

See also

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References

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  1. ^abcd"NGC 527".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-12-09.
  2. ^abcdefg"Revised NGC Data for NGC 527".spider.seds.org. Retrieved2017-10-05.
  3. ^ab"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2017-10-05.
  4. ^abcAn object's distance from Earth can be determined usingHubble's law:v=Ho is Hubble's constant (70±5 (km/s)/Mpc). The relative uncertainty Δd/d divided by the distance is equal to the sum of the relative uncertainties of the velocity andv=Ho
  5. ^abc"New General Catalog Objects: NGC 500 - 549".cseligman.com. Retrieved2017-10-16.
  6. ^"astronomy-mall.com/Adventures.In.Deep.Space/NGC%201-7840%20complete.htm".

External links

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Wikimedia Commons has media related toNGC 527.


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