UGC 4881 (also known as The Grasshopper) is a pair of interacting galaxies, UGC 4881A and UGC 4881B.[1] They are located in the constellation Lynx, some 500 million light-years away. UGC 4881, the brighter, is a peculiar spiral galaxy. It has been heavily documented by the Hubble Space Telescope, and is cataloged in the Atlas of Peculiar Galaxies.[2][3]
UGC 4881 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Lynx |
Right ascension | 09 15 55.5 |
Declination | +44 19 58 |
Redshift | 0.039184 |
Heliocentric radial velocity | 11,919 km/s |
Distance | 500 Mly |
Other designations | |
PGC 26132, MCG +08-17-065, Arp 55 |
Etymology
editThis section needs additional citations for verification. (May 2024) |
UGC 4881 was first given the nickname "The Grasshopper" by astrophysicist Dr. Boris Vorontsov-Velyaminov in a 1977 paper[2][unreliable source?] due to its resemblance to a grasshopper larva. It has also been informally called the "Shrimp galaxy" due to the curvature of the arm resembling a shrimp.[citation needed]
Morphology
editThe two galaxy cores are the two brightest regions in the object. The cores of each merging galaxy are separated and distinct, but the disks of the galaxies have started to merge. Intense star formation is occurring, as seen by the bright blue line of clusters along the grasshopper's "tail". Three other faint galaxies are visible near UGC 4881 and form a group with it.[4]
Formation
editUGC 4881 is believed to be in the process of merging, but the discs of the parent galaxies are overlapping while the cores are separated. A supernova exploded inside of UGC 4881 in 1999 and the galaxy is in the beginning of star formation.[4]
See also
editReferences
edit- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-20.
- ^ a b Iovene, Salvatore. "Arp 55". AstroBin. Retrieved 2024-04-19.
- ^ "Halton Arp's Atlas of Peculiar Galaxies". cseligman.com. Retrieved 2024-04-20.
- ^ a b information@eso.org. "UGC 4881". www.spacetelescope.org. Retrieved 2024-04-20.