Cannabaceae

NGC 5875
The spiral galaxy NGC 5875.
Observation data (J2000 epoch)
ConstellationBoötes
Right ascension15h 09m 13.16s[1]
Declination+52° 31′ 42.4″[1]
Redshift0.011695 [1]
Heliocentric radial velocity3506 ± 2 km/s[1]
Distance172.4 ± 12.1 Mly (52.87 ± 3.70 Mpc)[1]
Apparent magnitude (V)12.4[1]
Characteristics
TypeSAb?[1]
Size~116,800 ly (35.80 kpc) (estimated)[1]
Apparent size (V)2.3' x 1.2'[1]
Other designations
PGC 54095, UGC 9745, CGCG 274-027, MCG +09-25-027, IRAS 15077+5243, 2MASX J15091320+5231418[1]

NGC 5875 is an spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3585 ± 6 km/s, which corresponds to a Hubble distance of 52.87 ± 3.70 Mpc (∼173 million light-years).[1] It was discovered by German-British astronomer William Herschel on 1 May 1788.[2]

The SIMBAD database lists NGC 5875 as a Seyfert II Galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[3]

Two supernovae have been observed in NGC 5875: SN 2022oqm (type Ic-pec, mag 17.3)[4] and SN 2023ldh (type IIn, mag 20.7).[5] SN 2022oqm has been described as one of the brightest CaRTs (Calcium-rich Transients) known.[6]

See also

[edit]

References

[edit]
[edit]

One thought on “Cannabaceae

  1. Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
    View the detailed Guide of Psilotum nudum: Detailed Study Of Psilotum Nudum (Whisk Fern), Classification, Anatomy, Reproduction

Leave a Reply