In the Vinony graph
Within Vinony's link graph, NGC 91 is referenced by 983 other articles, and connects out to list of NGC objects (1–1000), NGC 241 and NGC 945.
Vinony files it under Andromeda (constellation), Astronomical objects discovered in 1866 and Discoveries by Herman Schultz (astronomer).
Its subject is documented across 36 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- *
- Distance
- 6,753 light-years
- Coordinates
- RA 5.4651° · Dec 22.3682°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Andromeda
- Right ascension
- 00 21 51.633
- Declination
- +22 ° 22 ′ 05.52 ″
via Wikipedia infobox
Wikidata facts
- Constellation
- Andromeda
- Distance from Earth
- 2006.0181
- Image
- NGC 0091 SDSS.jpg
Show 11 more facts
- epoch
- J2000.0
- right ascension component of proper motion
- -2.236
- right ascension
- 5.46510825421530
- declination
- 22.36822691580220
- parallax
- 0.4985
- catalog code
- Gaia DR2 2800700246182305408
- discoverer or inventor
- R. J. Mitchell
- time of discovery or invention
- 1854-10-26
- Commons category
- NGC 91
- apparent magnitude
- 14.4
- declination component of proper motion
- -3.148
via Wikidata · CC0
~1 min read
Encyclopedic overview
NGC 91 (PGC 3325956, GC 41, GC 5097, or NPD 68 22.9) is a star with an apparent magnitude of 14.4 in the constellation of Andromeda. The star is southwest of the galaxy NGC 90. Discovered in 1866 by Herman Schultz, there have been many arguments if this star exists or not. However, people have observed the star, and have confirmed that NGC 91 exists.
References
Excerpted from Wikipedia’s “NGC 91” article, available under the CC BY-SA 4.0 licence.