NGC 1439 explained

NGC 1439
Epoch:J2000
Type:E1[1]
Dist Ly:23.5 Mpc (76.6 Mly)
H Radial V:1668 ± 8 km/s
Appmag V:11.4
Size V:2.4 × 2.2
Constellation Name:Eridanus
Names:[2]

NGC 1439 is an elliptical galaxy located in constellation of Eridanus. Situated about 77 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 9 December 1784.

NGC 1439 has a Hubble classification of E1, which indicates it is an elliptical galaxy with no extensions. It is moving away from the Milky Way at a rate of 1,668 km/s. Its size on the night sky is 2.4' x 2.2' which is proportional to its real size of 54 000 ly.

NGC 1439 is an early-type galaxy. Despite their name, early-type galaxies are much older than spiral galaxies, and mostly comprise old, red-colored stars. Very little star formation occurs in these galaxies; the lack of star formation in elliptical galaxies appears to start at the center and then slowly propagates outward.[3]

Most of the galaxies like NGC 1439 are dust poor. However, NGC 1439 contains more dust than usual.[4]

Notes and References

  1. Book: Dunlop. Storm. Atlas of the Night Sky. Collins. 2005. 978-0-00-717223-8.
  2. NGC 1439. 2021-02-19.
  3. Web site: Colossal Ancient Galaxies Die from the Inside Out. space.com. Howell, Elizabeth. 2015. 5 March 2017.
  4. 10.1086/301440. The Central Gas Systems of Early-Type Galaxies Traced by Dust Features, Based on the Hubble Space Telescope WFPC2 Archival Images. 2000. Tomita. Akihiko. Aoki. Kentaro. Watanabe. Masaru. Takata. Tadafumi. Ichikawa. Shin-Ichi. The Astronomical Journal. 120. 1 . 123–130. astro-ph/0003431 . 9684945. 2000AJ....120..123T. free.