View source for NGC 1512

{{Short description|Galaxy in the constellation Horologium}}
{{Infobox Galaxy
| name = [[New General Catalogue|NGC]] 1512
| image = NGC1510, NGC 1512 - Noirlab2210a.jpg
| caption = NGC 1512 and [[NGC 1510]] imaged by the [[Cerro Tololo Inter-American Observatory]]
| epoch = [[J2000]]
| type = SB(r)ab<ref name="ned">{{cite web
  | title=NASA/IPAC Extragalactic Database
  | work=Results for NGC 1512
  | url=http://nedwww.ipac.caltech.edu/
  | access-date=2006-11-25 }}</ref>
| ra = {{RA|04|03|54.3}}<ref name="ned" />
| dec = {{DEC|-43|20|56}}<ref name="ned" />
| dist_ly = {{convert|11.6|Mpc|Mly|abbr=on|lk=on}} {{hub|0.73}}<ref name="ned-distance">{{cite web
  | title=NASA/IPAC Extragalactic Database
  | work=Results for NGC 1512, Co-Moving Radial Distance
  | url=http://nedwww.ipac.caltech.edu/
  | access-date=2014-12-18 }}</ref>
| z = 898 ± 3 km/[[second|s]]<ref name="ned" />
| appmag_v = 11.1<ref name="ned" />
| size_v = 8.9{{prime}} × 5.6{{prime}}<ref name="ned" />
| size = 213,140 [[Light-Year|ly]] (65.38 [[kiloparsec|kpc]]) (estimated)<ref name = ned/>
| constellation name = [[Horologium (constellation)|Horologium]]
| names = [[Principal Galaxies Catalogue|PGC]] 14391<ref name="ned" />
}}

'''NGC 1512''' is a [[barred spiral galaxy]] approximately [[1 E22 m|38 million]] [[light-year]]s away from Earth<ref name="ned-distance" /> in the [[constellation]] [[Horologium (constellation)|Horologium]]. The galaxy displays a double ring structure, with a (nuclear) ring around the galactic nucleus and an (inner) further out in the main disk. The galaxy hosts an extended UV disc with at least 200 clusters with recent star formation activity.<ref name="Monthly400" /> NGC 1512 is a member of the [[Dorado Group]].<ref name="Maiaetal1989">{{Cite journal
 | bibcode = 1989ApJS...69..809M
 | date = April 1989
 | journal = Astrophysical Journal Supplement Series
 | volume = 69
 | pages = 809&ndash;829
 | doi = 10.1086/191328
 | title = A catalog of southern groups of galaxies
 | author = Maia, M. A. G. | author2 =da Costa, L. N. | author3 =Latham, David W.
 | doi-access = free
 }}</ref>

==Gravitational interaction with NGC 1510==
Gravitational tidal forces of NGC 1512 are influencing nearby [[dwarf galaxy|dwarf]] [[lenticular galaxy]] [[NGC 1510]]. The two galaxies are separated by only ~5 arcmin (13.8 kpc),<ref name=Monthly400>{{cite journal
 |last1=Koribalski |first1=Bärbel S. 
 |last2=López-Sánchez |first2= Ángel R. 
 |date=2009
 |title=Gas dynamics and star formation in the galaxy pair NGC 1512/1510
 |journal=[[Monthly Notices of the Royal Astronomical Society]]
 |volume=400 |issue=4 |pages=21
 |doi=10.1111/j.1365-2966.2009.15610.x 
|doi-access=free 
 |arxiv=0908.4128|bibcode=2009MNRAS.400.1749K|s2cid=9329781 
 }}</ref> and are in the process of a lengthy merger which has been going on for 400 million years.<ref name=david>{{cite web|title=Galactic David and Goliath|url=https://www.spacetelescope.org/news/heic1712/|website=www.spacetelescope.org|access-date=27 November 2017|archive-url=https://web.archive.org/web/20171201032836/https://www.spacetelescope.org/news/heic1712/|archive-date=1 December 2017|url-status=dead}}</ref> At the end of this process NGC 1512 will have cannibalised its smaller companion.<ref name=esa>{{cite web|title=NGC 1512 and NGC 1510|url=http://sci.esa.int/hubble/59356-ngc-1512-and-ngc-1510/|website=sci.esa.int|access-date=27 November 2017|archive-url=https://web.archive.org/web/20171201032832/http://sci.esa.int/hubble/59356-ngc-1512-and-ngc-1510/|archive-date=1 December 2017|url-status=dead}}</ref>

Interaction between these two galaxies has triggered star formation activity in the outskirts of the disc and enhanced the tidal distortion in the arms of the NGC 1512. The interaction seems to occur in the north-western areas of the system because of the broadening of the H i arm and the spread of the UV-rich star clusters in this region.<ref name="Monthly400" />

==Gallery==
<gallery>
NGC 1512 and NGC 1510.jpg|NGC 1512 and its companion the dwarf galaxy [[NGC 1510]].<ref name=david />
Ngc1512 nasajpl.jpg|An [[ultraviolet]] image of [[NGC 1510]] and NGC 1512 taken with [[GALEX]].  The image shows that NGC 1512 has spiral arms that extend well beyond its optical disk.  Credit:GALEX/[[NASA]]/[[JPL]]-[[Caltech]].
NGC 1512 (2).jpg|The galaxy seen by the [[Hubble Space Telescope]].
NGC 1512 (weic2403i).jpg|NGC 1512 seen by the [[James Webb Space Telescope]].
NGC 1512.jpg|The nuclear ring of NGC 1512 as imaged by the [[Hubble Space Telescope]] (HST).<br/>Credit: HST/[[NASA]]/[[ESA]].
</gallery>

==See also==
* [[NGC 4314]]
* [[Messier 94]]

==References==
{{reflist}}

==External links==
{{commons category}}
* {{APOD |date=6 June 2001 |title=A Panchromatic View}}
* [https://web.archive.org/web/20010605122858/http://www.space.com/scienceastronomy/astronomy/hubble_galaxy_010531.html '''SPACE.com''': Baby Stars Clean House Quickly]

{{Ngc20}}
{{Horologium (constellation)}}

{{DEFAULTSORT:NGC 1512}}
[[Category:Barred spiral galaxies]]
[[Category:Interacting galaxies]]
[[Category:Dorado Group]]
[[Category:Horologium (constellation)]]
[[Category:NGC objects|1512]]
[[Category:Principal Galaxies Catalogue objects|014391]]
[[Category:Ring galaxies]]


{{Spiral-galaxy-stub}}