In the Vinony graph
Vinony's link graph records 376 inbound references to NGC 1701, and connects out to list of NGC objects (1001–2000), Caelum and epoch.
It is catalogued under topics including Astronomical objects discovered in 1834, Caelum and Discoveries by John Herschel.
Vinony links it to 29 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- AG?
- Distance
- 3,345 light-years
- Redshift
- z = 0.019564756578674514
- Coordinates
- RA 73.9631° · Dec -29.8835°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Caelum
- Right ascension
- 04 55 51.1486
- Declination
- −29 ° 53 ′ 00.980 ″
- Redshift
- 0.019 467 ± 0.000 0800
- Heliocentric radial velocity
- 5,836 ± 24 km/s
- Distance
- 280.8 ± 19.7 Mly (86.08 ± 6.05 Mpc )
- Surface brightness
- 22.65 mag/arcsec
- Type
- (R)SA(r)b
- Size
- ~170,500 ly (52.28 kpc ) (estimated)
- Apparent size v
- 1.2′ × 0.9′
via Wikipedia infobox
Wikidata facts
- Instance of
- spiral galaxy
- Constellation
- Caelum
- Image
- NGC 1701 legacy dr10.jpg
Show 11 more facts
- epoch
- J2000.0
- catalog code
- Gaia DR2 4876614964344897792
- Commons category
- NGC 1701
- galaxy morphological type
- Sa
- time of discovery or invention
- 1834-11-06
- discoverer or inventor
- John Frederick William Herschel
- apparent magnitude
- 9.888
- right ascension
- 73.96314632918160
- declination
- -29.88355077719010
- radial velocity
- 5808
- redshift
- 0.019373
Sources (2)
via Wikidata · CC0
~1 min read
Encyclopedic overview
NGC 1701, also known as the Trekkie Galaxy, is a large unbarred spiral galaxy located in the constellation Caelum. Its speed relative to the cosmic microwave background is 5,836 ± 24 km/s, which corresponds to a Hubble distance of 86.1 ± 6.0 Mpc (~281 million ly). It was discovered by British astronomer John Herschel on 6 November 1834.
The luminosity class of NGC 1701 is II and it has a broad HI line.
Excerpted from Wikipedia’s “NGC 1701” article, available under the CC BY-SA 4.0 licence.
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