NGC 1325
Sign in to savebarred spiral galaxy in the constellation Eridanus
In the Vinony graph
Vinony's link graph records 491 inbound references to NGC 1325, and connects out to list of NGC objects (1001–2000), epoch and NGC 1974.
It sits within the topics Barred spiral galaxies, Eridanus (constellation) and Eridanus Group.
Vinony links it to 31 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- EmG
- Redshift
- z = 0.005358721677222844
- Coordinates
- RA 51.1066° · Dec -21.5441°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Eridanus
- Right ascension
- 03 25.576
- Declination
- −21 ° 32 ′ 38.61 ″
- Heliocentric radial velocity
- 1,588
- Distance
- 75.0 Mly (23.01 Mpc ) h , 0.73
- Group or cluster
- Eridanus Cluster
- Type
- SBbc
- Apparent size v
- 4.47 ′ × 1.66 ′
- Notable features
- Flocculent spiral galaxy
via Wikipedia infobox
Wikidata facts
- Instance of
- spiral galaxy
- Constellation
- Eridanus
- Distance from Earth
- 19
- Image
- NGC 1325 DSS.jpg
Show 11 more facts
- catalog code
- LEDA 12737
- discoverer or inventor
- William Herschel
- galaxy morphological type
- Sb
- Commons category
- NGC 1325
- time of discovery or invention
- 1798-00-00
- redshift
- 0.005300
- apparent magnitude
- 8.627
- right ascension
- 51.10656800397020
- declination
- -21.54405749430540
- radial velocity
- 1596
- epoch
- J2000.0
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
NGC 1325 is a flocculent spiral galaxy situated in the constellation of Eridanus. Located about 75 million light years away, it is a member of the Eridanus Cluster of galaxies, a cluster of about 200 galaxies. It was discovered by William Herschel on 19 December 1799.
NGC 1325 has a Hubble classification of SBbc, which indicates it is a barred spiral galaxy with moderately wound arms. Its angular size on the night sky is 4.5' x 1.7'. The disk of the galaxy is inclined at an angle of 71° with the main axis aligned along a position angle of 232°. The rotation curve for the galaxy is flat across much of the radius from the core. The galaxy is moving away from the Milky Way with a heliocentric radial velocity of 1,588 km/s.
Excerpted from Wikipedia’s “NGC 1325” article, available under the CC BY-SA 4.0 licence.
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