NGC 116
Galaxy NGC 116 |
|
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NGC 116 with LEDA 1015126 (r) SDSS image | |
AladinLite | |
Constellation | whale |
Position equinox : J2000.0 , epoch : J2000.0 |
|
Right ascension | 00 h 27 m 05.2 s |
declination | -07 ° 40 ′ 06 ″ |
Appearance | |
Morphological type | SB? (R?) 0+: |
Brightness (B-band) | 14.54 mag |
Angular expansion | 0.6 ′ × 0.3 ′ |
Physical data | |
Redshift | 0.025261 ± 0.000080 |
Radial velocity | 7573 ± 24 km / s |
Stroke distance v rad / H 0 |
(341 ± 24) x 10 6 ly (104.7 ± 7.3) Mpc |
history | |
discovery | Gaspare Ferrari |
Discovery date | 1865 |
Catalog names | |
NGC 116 • PGC 1671 • MCG -01-02-017 • 2MASX J00270522-0740059 • GC 5101 • GALEX ASC J002705.26-074005.4 • USGC S012 NED02 |
NGC 116 is a spiral galaxy of Hubble type SB? in the constellation whale south of the ecliptic . It is estimated to be 341 million light years away from the Milky Way and has a diameter of around 60,000 ly.
In the same area of the sky is the galaxy NGC 107 .
discovery
The galaxy NGC 116 was discovered in 1865 by the Italian astronomer Gaspare Stanislao Ferrari . However, with this identification there are doubts as to whether it is actually the object, as there is nothing in the position specified by Ferrari, so that the object is considered lost or not present in other catalogs. Since the galaxy PGC 1671 is the brightest galaxy "near" the position and is almost exactly north of it, it could be a position error. Without a description, apart from "very weak" and the major flaw in its position, it is very unclear whether the identification as NGC 116 is reasonable, let alone probable.
Web links
Individual evidence
- ^ Aladin Lite
- ↑ a b c d e NASA / IPAC EXTRAGALACTIC DATABASE
- ↑ SIMBAD Astronomical Database
- ↑ Seligman