Balkespiralgalaxie am Stärebild Cetus From Wikipedia, the free encyclopedia
Den NGC 66 ass eng Balkespiralgalaxie am Stärebild Cetus.
 Foto, opgeholl vum 2MASS. | |
| Stärebild |
Cetus (Cet) |
|---|---|
| Positioun fir d'Equinoxe J2000.0 | |
| Rektaszensioun | 00h 19m 04.94s |
| Deklinatioun | - 22° 56' 11"[1] |
| Ausgesinn | |
| Hubble-Sequenz | SB(r)b pec HII[1] |
| Visuell Magnitude | +13,4[2] mag |
| Visuell Magnitude (B-Band) | +14,2[2] mag |
| Wénkelduerchmiesser | 1.2 × 0.48[1] |
| Flächenhellegkeet mag/arcmin² | +13,1[2] |
| Physikalesch Donnéeën | |
| Routverrécklung | (25364 ± 33) ∙ 10-6[1] |
| Radialvitess | (+7604 ± 10) |
| Geschicht | |
| Entdecker | Frank Muller |
| Entdeckungsdatum | 1886 |
| Katalog- an Entdeckerbezeechnungen | |
| AM | 0016-231 |
| IRAS | 00165-2312 |
| MCG | -04-02-002 |
| NGC | 66 |
| PGC | 1236 |
| ESO | 473-10 |
D'Galaxie NGC 66 gouf am Joer 1886 vum amerikaneschen Astronom Frank Muller entdeckt.
| Commons: NGC 66 – Biller, Videoen oder Audiodateien |
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