NGC 5416
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| NGC 5416 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 14h 02m 11.3153s[1] |
| Declination | +09° 26′ 24.350″[1] |
| Redshift | 0.020811±0.00000900[1] |
| Distance | 261.42 ± 8.13 Mly (80.152 ± 2.492 Mpc)[1] |
| Apparent magnitude (B) | 13.6[1] |
| Surface brightness | 22.79 mag/arcsec^2 |
| Characteristics | |
| Type | Scd[1] |
| Size | ~114,100 ly (34.97 kpc) (estimated)[1] |
| Apparent size (V) | 1.37′ × 0.75′[1] |
| Other designations | |
| IRAS 13597+0940, UGC 8944, MCG +02-36-014, PGC 49991, CGCG 074-052 | |
NGC 5416 is a spiral galaxy and radio galaxy[2] located in the constellation Boötes. Its speed relative to the cosmic microwave background is 6,499 ± 18 km/s, which corresponds to a Hubble distance of 95.9 ± 6.7 Mpc (~313 million ly).[1] NGC 5416 was discovered by German-British astronomer William Herschel on 19 March 1784.[3]
The luminosity class of NGC 5416 is III-IV and it has a broad HI line.[1] According to the SIMBAD database, NGC 5416 is a radio galaxy.[2]
To date, 25 non-redshift measurements yield a distance of 80.152 ± 2.492 Mpc (~261 million ly),[4] which is within the Hubble distance values. Note that it is with the average value of independent measurements, when they exist, that the NASA/IPAC database calculates the diameter of a galaxy and that consequently the diameter of NGC 5416 could be approximately 41.8 kpc (~136,000 ly) if we used the Hubble distance to calculate it.[5]
Supernova
One supernova has been observed in NGC 5416: SN 2025trg (Type II, mag. 19.6808) was discovered by the Zwicky Transient Facility on 11 August 2025.[7]