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 519
NGC 519
NGC 519 as seen on SDSS
Observation data (J2000[1] epoch)
ConstellationCetus[2]
Right ascension01h 24m 28.6s[3]
Declination−01° 38′ 29″[3]
Redshift0.017756 ± 0.000260[1]
Heliocentric radial velocity(5276 ± 78) km/s[1]
Distance242 Mly[4]
Apparent magnitude (V)14.4[2]
Apparent magnitude (B)15.4[2]
Characteristics
TypeE[2]
Apparent size (V)0.5' × 0.3'[2]
Other designations
PGC 5182, MGC +00-04-116, 2MASS J01242863-0138284[1][5]

NGC 519, also occasionally referred to as PGC 5182, is an elliptical galaxy located approximately 242 million light-years from the Solar System[4] in the constellation Cetus.[2] It was discovered on 20 November 1886 by astronomer Lewis Swift.[5]

YouTube Encyclopedic

  • 1/5
    Views:
    3 527
    1 244
    527
    810
    520
  • Neutron Star Binary Mergers
  • The Heart Nebula Captured in Color...Finally
  • Close Up View of Globular Star Cluster NGC 6362
  • Helix Nebula Complete, Working on M17 & Bubble
  • Hubble Spots Super Nova

Transcription

Observation history

Swift discovered the object along with NGC 530, 538 and 557 using a 16-inch refractor telescope at the Warner Observatory.[6] It was later catalogued by John Louis Emil Dreyer in the New General Catalogue, where the galaxy was described as "most extremely faint, very small, round, very difficult".[5]

Description

The galaxy appears very dim in the sky as it only has an apparent visual magnitude of 14.4. It can be classified as type E using the Hubble Sequence.[2] The object's distance of roughly 240 million light-years from the Solar System can be estimated using its redshift and Hubble's law.[4]

NGC 519 (SDSS)

See also

References

  1. ^ a b c d "NGC 519". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-12-09.
  2. ^ a b c d e f g "Revised NGC Data for NGC 519". 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 c 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. ^ "astronomy-mall.com/Adventures.In.Deep.Space/NGC%201-7840%20complete.htm".

External links

This page was last edited on 23 June 2023, at 21:10
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.