NGC 1544
| Galaxie NGC 1544 | |
|---|---|
 | |
| AladinLite | |
| Sternbild | Kepheus |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 05h 02m 36,1s[1] |
| Deklination | +86° 13′ 20″[1] |
| Erscheinungsbild | |
| Morphologischer Typ | S0[1][2] |
| Helligkeit (visuell) | 13,6 mag[2] |
| Helligkeit (B-Band) | 14,5 mag[2] |
| Winkelausdehnung | 1,3′ × 0,9′[2] |
| Positionswinkel | 130°[2] |
| Flächenhelligkeit | 13,6 mag/arcmin²[2] |
| Physikalische Daten | |
| Rotverschiebung | 0.013132 ± 0.000220[1] |
| Radialgeschwindigkeit | (3937 ± 66) km/s[1] |
| Hubbledistanz vrad / H0 | (183 ± 13) · 106 Lj (56,2 ± 4,0) Mpc [1] |
| Geschichte | |
| Entdeckung | Wilhelm Tempel |
| Entdeckungsdatum | 1876 |
| Katalogbezeichnungen | |
| NGC 1544 • UGC 3160 • PGC 16608 • CGCG 361-011/362-004/370-001 • MCG +14-03-006 • 2MASX J05023656+8613203 • | |
NGC 1544 ist eine Galaxie vom Hubble-Typ S im Sternbild Kepheus am Nordsternhimmel. Sie ist schätzungsweise 183 Millionen Lichtjahre von der Milchstraße entfernt.
Das Objekt wurde im Jahre 1876 von Wilhelm Tempel entdeckt.[3]
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Auf dieser Seite verwendete Medien
NGC 1544 PanS.jpg
Autor/Urheber: Donald Pelletier, Lizenz: CC BY-SA 4.0
Image created using the Aladin Sky Atlas software from the Strasbourg Astronomical Data Center and
Autor/Urheber: Donald Pelletier, Lizenz: CC BY-SA 4.0
Image created using the Aladin Sky Atlas software from the Strasbourg Astronomical Data Center and
Pan-STARRS ([https://panstarrs.stsci.edu/ Panoramic Survey Telescope And Rapid Response System)
public data.
Cepheus constellation map.png
Autor/Urheber: Copyright © 2003 Torsten Bronger., Lizenz: CC-BY-SA-3.0
It was created by Torsten Bronger using the program PP3 on 2003/08/18. At PP3's homepage, you also get the input scripts necessary for re-compiling the map.
Autor/Urheber: Copyright © 2003 Torsten Bronger., Lizenz: CC-BY-SA-3.0
It was created by Torsten Bronger using the program PP3 on 2003/08/18. At PP3's homepage, you also get the input scripts necessary for re-compiling the map.
The yellow dashed lines are constellation boundaries, the red dashed line is the ecliptic, and the shades of blue show Milky Way areas of different brightness. The map contains all Messier objects, except for colliding ones. The underlying database contains all stars brighter than 6.5. All coordinates refer to equinox 2000.0.
The map is calculated with the equidistant azimuthal projection (the zenith being in the center of the image). The north pole is to the top. The (horizontal) lines of equal declination are drawn for 0°, ±10°, ±20° etc. The lines of equal rectascension are drawn for all 24 hours. Towards the rim there is a very slight magnification (and distortion).