NGC 4030
| Galaxie NGC 4030 | |
|---|---|
 | |
| NGC 4030[1] ESO | |
| AladinLite | |
| Sternbild | Jungfrau |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 12h 00m 23,627s[2] |
| Deklination | -01° 06′ 00,34″[2] |
| Erscheinungsbild | |
| Morphologischer Typ | SA(s)bc / HII[2][3] |
| Helligkeit (visuell) | 10,6 mag[3] |
| Helligkeit (B-Band) | 11,4 mag[3] |
| Winkelausdehnung | 4,2′ × 3,2′[3] |
| Positionswinkel | 27°[3] |
| Flächenhelligkeit | 13,3 mag/arcmin²[3] |
| Physikalische Daten | |
| Zugehörigkeit | NGC-4030-Gruppe (Virgo-II-Gruppe) LGG 264[2][4] |
| Rotverschiebung | 0.004887 ± 0.000013[2] |
| Radialgeschwindigkeit | (1465 ± 4) km/s[2] |
| Hubbledistanz vrad / H0 | (60 ± 4) · 106 Lj (18,5 ± 1,3) Mpc [2] |
| Durchmesser | 70.000 Lj |
| Geschichte | |
| Entdeckung | Wilhelm Herschel |
| Entdeckungsdatum | 1. Januar 1786 |
| Katalogbezeichnungen | |
| NGC 4030 • UGC 6993 • PGC 37845 • CGCG 013-033 • MCG +00-31-016 • IRAS 11578-0049 • 2MASX J12002364-0105598 • GC 2663 • H I 121 • h 1048 • HIPASS J1200-01 • WISEA J120023.63-010600.1 • EVCC 72 | |
NGC 4030 ist eine Spiralgalaxie mit ausgedehnten Sternentstehungsgebieten vom Hubble-Typ Sbc im Sternbild Jungfrau, etwa 1° südlich vom Herbstpunkt. Sie ist schätzungsweise 60 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 80.000 Lichtjahren.
Im selben Himmelsareal befinden sich u. a. die Galaxien IC 753 und IC 754.
Am 19. Februar 2007 wurde hier SN 2007aa, eine Supernova Typ IIP, beobachtet.[5]
Das Objekt wurde am 1. Januar 1786 von William Herschel entdeckt.[6]
NGC 4030-Gruppe (LGG 264)
| Galaxie | Alternativname | Entfernung/Mio. Lj |
|---|---|---|
| NGC 4030 | PGC 37845 | 60 |
| PGC 37710 | UGC 6970 | 61 |
| PGC 37737 | UGC 6978 | 64 |
| PGC 37914 | UGC 7000 | 62 |
Weblinks
Commons: NGC 4030 – Sammlung von Bildern, Videos und Audiodateien
- SIMBAD Astronomical Database
- ESO: HAWK-I image of NGC 4030 (engl.)
Einzelnachweise
Auf dieser Seite verwendete Medien
HAWK-I NGC 4030.jpg
Autor/Urheber: ESO/P. Grosbøl, Lizenz: CC BY 4.0
This spiral galaxy, NGC 4030, lies about 75 million light-years from Earth, in the constellation of Virgo. In 2007 Takao Doi, a Japanese astronaut who doubles as an amateur astronomer, spotted a supernova — a stellar explosion that is briefly almost as bright as its host galaxy — going off in this galaxy. The image was made in infrared light with the HAWK-I camera on ESO’s Very Large Telescope at Paranal Observatory in Chile. HAWK-I is one of the most powerful infrared imagers in the world, and this is one of the sharpest and most detailed pictures of this galaxy ever taken from Earth. The filters used were Y (shown here in blue), J (in green), H (in orange), and K (in red). The field of view of the image is about 6.4 arcminutes across.
Autor/Urheber: ESO/P. Grosbøl, Lizenz: CC BY 4.0
This spiral galaxy, NGC 4030, lies about 75 million light-years from Earth, in the constellation of Virgo. In 2007 Takao Doi, a Japanese astronaut who doubles as an amateur astronomer, spotted a supernova — a stellar explosion that is briefly almost as bright as its host galaxy — going off in this galaxy. The image was made in infrared light with the HAWK-I camera on ESO’s Very Large Telescope at Paranal Observatory in Chile. HAWK-I is one of the most powerful infrared imagers in the world, and this is one of the sharpest and most detailed pictures of this galaxy ever taken from Earth. The filters used were Y (shown here in blue), J (in green), H (in orange), and K (in red). The field of view of the image is about 6.4 arcminutes across.
