NGC 4440 explained
NGC 4440 |
Epoch: | J2000 |
Type: | SB(rs)a[1] |
Dist Ly: | 56,400,000 ly[2] |
Group Cluster: | Virgo Cluster |
Z: | 0.002415/724 km/s |
Appmag V: | 12.70 |
Size V: | 1.9 x 1.5 |
Constellation Name: | Virgo |
Names: | PGC 40927, UGC 7581, VCC 1047 |
Size: | ~30,550 ly (estimated) |
NGC 4440 is a barred spiral galaxy located about 55 million light-years away[3] in the constellation of Virgo.[4] NGC 4440 was discovered by astronomer William Herschel on April 17, 1784.[5] It is a member of the Virgo Cluster.[6]
Physical characteristics
NGC 4440 has a strong bar in its structure. Surrounding the bar, there are two very open spiral arms.[7]
See also
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 4440 . 2017-09-30.
- Web site: parsecs to lightyears conversion. 2017-09-30.
- Web site: Your NED Search Results. ned.ipac.caltech.edu. 2017-09-30.
- Web site: Galaxy NGC 4440 - Barred Spiral Galaxy in Virgo Constellation · Deep Sky Objects Browser. Rojas. Sebastián García. DSO Browser. en. 2017-09-30. 2017-10-01. https://web.archive.org/web/20171001074310/https://dso-browser.com/deep-sky/5486/ngc-4440/galaxy. dead.
- Web site: New General Catalog Objects: NGC 4400 - 4449. cseligman.com. en-US. 2017-09-30.
- Web site: Detailed Object Classifications. ned.ipac.caltech.edu. 2017-09-30.
- Web site: NGC 4440 - SB(rs)a. The De Vaucouleurs Atlas of Galaxies. 2017-09-30. 2019-03-02. https://web.archive.org/web/20190302232131/http://kudzu.astr.ua.edu/devatlas/NGC_4440______g___________.html. dead.