NGC 2340
Galaxy in the constellation Lynx
From Wikipedia, the free encyclopedia
NGC 2340 is a large elliptical galaxy in the constellation of Lynx. Its velocity with respect to the cosmic microwave background is 6,008±9 km/s, which corresponds to a Hubble distance of 289.0 ± 20.3 Mly (88.61 ± 6.21 Mpc).[1] However, six non-redshift measurements give a farther mean distance of 315.77 ± 44.34 Mly (96.817 ± 13.596 Mpc).[2] It was discovered by German-British astronomer William Herschel on 9 February 1788.[3]
| NGC 2340 | |
|---|---|
NGC 2340 imaged by Pan-STARRS | |
| Observation data (J2000 epoch) | |
| Constellation | Lynx |
| Right ascension | 07h 11m 10.7950s[1] |
| Declination | +50° 10′ 29.075″[1] |
| Redshift | 0.019764±0.0000250[1] |
| Heliocentric radial velocity | 5,925±7 km/s[1] |
| Distance | 315.77 ± 44.34 Mly (96.817 ± 13.596 Mpc)[1] |
| Apparent magnitude (V) | 12.7[1] |
| Characteristics | |
| Type | E[1] |
| Size | ~263,000 ly (80.64 kpc) (estimated)[1] |
| Apparent size (V) | 1.8′ × 1.2′[1] |
| Other designations | |
| 2MASX J07111080+5010288, UGC 3720, MCG +08-13-096, PGC 20338, CGCG 234-091[1] | |
NGC 2340 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[4][5]
Abell 569 member
Supernova
One supernova has been observed in NGC 2340:
- SN 2025hlm (Type Ia-91bg-like, mag. 19.7586) was discovered by the Zwicky Transient Facility on 16 April 2025.[7]