To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

NGC 502
NGC 502
SDSS view of NGC 502
Observation data (J2000[1] epoch)
ConstellationPisces[2]
Right ascension01h 22m 55.5s[3]
Declination+09° 02′ 57″[3]
Redshift0.008279 ± 0.000163[1]
Heliocentric radial velocity(2472 ± 49) km/s[1]
Distance113 Mly[4]
Apparent magnitude (V)12.7[2]
Apparent magnitude (B)13.7[2]
Characteristics
TypeS0[2]
Apparent size (V)1.1' × 1.0'[2]
Other designations
GC 293, 2MASS J01225553+0902570, UGC 922, PGC 5034 [1][5]

NGC 502, also occasionally referred to as PGC 5034 or UGC 922, is a lenticular galaxy in the constellation Pisces.[2] It is located approximately 113 million light-years from the Solar System[4] and was discovered on 25 September 1862 by German astronomer Heinrich Louis d'Arrest.[5] When the Morphological Catalogue of Galaxies was published between 1962 and 1974, the identifications of NGC 502 and NGC 505 were reversed. In reality, NGC 502 is equal to MGC +01-04-041 and not MCG +01-04-043 as noted in the catalogue.[6]

YouTube Encyclopedic

  • 1/5
    Views:
    1 040
    11 181
    3 022
    5 872
    3 021
  • Andromeda (constellation)
  • Um Oceano no Coração de Plutão - Space Today TV Ep.503
  • Capturing the Whale and Hockey Stick Galaxies
  • Armchair Astrophysics: Finding Physics Far and Wide
  • Astronomy Cast Ep. 499: What is the proposed Hubble-Lemaitre Law?

Transcription

Observation history

Arrest discovered NGC 502 using an 11" reflecting telescope in Copenhagen. His position, which he measured on four separate nights, matches with both UGC 922 and PGC 5034.[6] John Louis Emil Dreyer, creator of the New General Catalogue, described the galaxy as "considerably bright, small, round, brighter middle and nucleus".[5]

NGC 502 (SDSS)

See also

References

  1. ^ a b c d "NGC 502". Retrieved 2017-12-09.
  2. ^ a b c d e f "Revised NGC Data for NGC 502". spider.seds.org. Retrieved 2017-10-05.
  3. ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-10-05.
  4. ^ a b An object's distance from Earth can be determined using Hubble'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 and v=Ho
  5. ^ a b c "New General Catalog Objects: NGC 500 - 549". cseligman.com. Retrieved 2017-10-16.
  6. ^ a b "astronomy-mall.com/Adventures.In.Deep.Space/NGC%201-7840%20complete.htm".

External links


This page was last edited on 6 April 2022, at 15:45
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.