NGC 800
| Galaxie NGC 800 | |
|---|---|
 | |
| Aufnahme mittels des Very-Large-Telescope-Instruments FORS. (NGC 799 in der Bildmitte, darüber NGC 800) | |
| AladinLite | |
| Sternbild | Walfisch |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 02h 02m 11,8s[1] |
| Deklination | -00° 07′ 50″[1] |
| Erscheinungsbild | |
| Morphologischer Typ | SA(rs)c:[1][2] |
| Helligkeit (visuell) | 13,1 mag[2] |
| Helligkeit (B-Band) | 13,8 mag[2] |
| Winkelausdehnung | 1′ × 0,9′[2] |
| Positionswinkel | 10°[2] |
| Flächenhelligkeit | 12,8 mag/arcmin²[2] |
| Physikalische Daten | |
| Rotverschiebung | 0,019899 ± 0,000075[1] |
| Radialgeschwindigkeit | 5966 ± 22 km/s[1] |
| Hubbledistanz vrad / H0 | (268 ± 19) · 106 Lj (82,2 ± 5,8) Mpc [1] |
| Geschichte | |
| Entdeckung | Lewis Swift |
| Entdeckungsdatum | 9. Oktober 1885 |
| Katalogbezeichnungen | |
| NGC 800 • UGC 1526 • PGC 7740 • CGCG 387-028 • MCG +00-06-024 • IRAS 01596-0021 • KUG 0159-003 • 2MASX J02021183-0007495 • NSA 062408 • HOLM 54B • KPG 52A | |
NGC 800 ist eine Spiralgalaxie vom Hubble-Typ Sc im Sternbild Walfisch südlich der Ekliptik. Sie ist rund 268 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 80.000 Lj. Gemeinsam mit NGC 799 bildet sie das gravitativ gebundenes Galaxienpaar Holm 54 oder KPG 52.
Das Objekt wurde am 9. Oktober 1885 von dem US-amerikanischen Astronomen Lewis Swift mit einem 41-cm-Teleskop entdeckt.[3]
Weblinks
- SIMBAD Astronomical Database
- ESO: Die Ruhe vor dem Sturm
- astronews.com: Bild des Tages 12. August 2013
Einzelnachweise
Auf dieser Seite verwendete Medien
Autor/Urheber: ESO, Lizenz: CC BY 4.0
This beautiful image portrays the galaxies NGC 799 (below) and NGC 800 (above) located in the constellation of Cetus (The Whale). This pair of galaxies was first observed by the American astronomer Lewis Swift back in 1885.
Located at a distance of about 300 million light-years, our face-on view allows us to clearly appreciate their shapes. Like the Milky Way — our galaxy — these objects are both spiral galaxies, with characteristic long arms winding towards a bright bulge at the centre. In the prominent spiral arms, a large number of hot, young, blue stars are forming in clusters (tiny blue dots seen in the image) whereas in the central bulge a large group of cooler, redder, old stars are packed into a compact, almost spherical region.
At first glance, these galaxies look rather similar, but the devil is in the detail. Apart from the obvious difference in size, only NGC 799 has a bar structure, extending from its central bulge, and the spiral arms wind out from the ends of the bar. Galactic bars are thought to act as a mechanism that channels gas from the spiral arms to the centre, intensifying star formation. A supernova was also observed in NGC 799 in 2004, and was given the name SN2004dt.
Another interesting differentiating feature is the number of spiral arms. The small NGC 800 has three bright, knotty spiral arms, whilst NGC 799 only has two relatively dim, but broad spiral arms. These start at the end of the bar and wrap nearly completely around the galaxy forming a structure that looks almost like a ring.
While it might seem that this image depicts two impressive close spiral galaxies coexisting in an everlasting peace, nothing can be further than the truth. We could be just witnessing the calm before the storm. We don’t know exactly what the future will bring, but typically, when two galaxies are close enough, they interact over hundreds of millions of years by means of gravitational disturbances. In some cases, only minor interactions occur, causing shape distortions, but sometimes galaxies collide, merging to form a single, new and larger galaxy.
The image was obtained using the FORS1 instrument on the 8.2-metre ESO Very Large Telescope (VLT) atop Cerro Paranal, Chile. It combines exposures taken through three filters (B, V, R).
Five asteroids can also be seen — can you find them all? The asteroids moved between the different exposures leaving colourful streaks in the image.