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NGC 114 Kuckt och | Um Spaweck | Referenzen NavigatiounsmenüSIMBAD QueryArtikel a Biller zu NGC 114 op wikisky.orgNASA/IPAC Extragalactic DatabaseSIMBAD QueryNASA/IPAC Extragalactic DatabaseStudents for the Exploration and Development of Spaceä

NGC 106NGC 107NGC 108NGC 109NGC 110NGC 111NGC 112NGC 113NGC 115NGC 116NGC 117NGC 118NGC 119NGC 120NGC 121NGC 122


NGC-Objete vun 1 bis 500Elliptesch Galaxien am NGC-KatalogStärebild CetusAstronomesch Objeten déi 1880 entdeckt goufen


lënsefërmeg GalaxisStärebildCetusSonnesystem27. September1880AstronomErnst Wilhelm Leberecht TempelSaturn 01.svg












NGC 114




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NGC 114

NGC114 - SDSS DR14.jpg
Stärebild
Cetus (Cet)
Positioun fir d'Equinoxe J2000.0
Rektaszensioun
00h 26m 58,41s
Deklinatioun
- 01° 47' 10,3"[1]
Ausgesinn
Hubble-Sequenz
SB(rs)0:[2]
Visuell Magnitude
13,3[3] mag

Visuell Magnitude
(B-Band)

14,3[3] mag
Wénkelduerchmiesser
1,0′ × 0,7′[1]

Flächenhellegkeet mag/arcmin²

12,5[3]
Physikalesch Donnéeën

Distanz (Lj)

MCP 51,8[2]
Routverrécklung
0,01231 ± 0,00023
Radialvitess
(3667 ± 70) [1]
Geschicht
Entdecker
E. W. L. Tempel
Entdeckungsdatum
27. September 1880
Katalog- an Entdeckerbezeechnungen
KUG
0024-020A
MCG
+00-02-027
NGC
114
NPM1G
-02.0005
PGC
1660
UGC
259
ZWG
383,14
2MASX
J00265821-0147100

Den NGC 114 ass eng lënsefërmeg Galaxis am Stärebild Cetus. Si läit ronn 185 Millioune Liichtjoer vun eisem Sonnesystem ewech an huet en Duerchmiesser vun zirka 50.000 Lj.[4]


Den NGC 114 gouf de 27. September 1880 vum däitschen Astronom Ernst Wilhelm Leberecht Tempel entdeckt.



Kuckt och |


Saturn 01.svgPortal Astronomie


  • Lëscht vun den NGC-Objeten

  • Index-Katalog

  • Messier-Katalog

  • NGC-Katalog


Um Spaweck |


  • SIMBAD Query

  • Artikel a Biller zu NGC 114 op wikisky.org


  • (en) NASA/IPAC Extragalactic Database



Referenzen



  1. ↑ 1,01,11,2 SIMBAD Query


  2. ↑ 2,02,1 NASA/IPAC Extragalactic Database


  3. ↑ 3,03,13,2 Students for the Exploration and Development of Space


  4. ↑ http://cseligman.com/text/atlas/ngc1.htm#114









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