NGC 3384
Galaxy in the constellation Leo
title: "NGC 3384" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["lenticular-galaxies", "barred-lenticular-galaxies", "m96-group", "leo-(constellation)", "ngc-objects", "ugc-objects", "principal-galaxies-catalogue-objects", "astronomical-objects-discovered-in-1784"] description: "Galaxy in the constellation Leo" topic_path: "science/astronomy" source: "https://en.wikipedia.org/wiki/NGC_3384" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0
::summary Galaxy in the constellation Leo ::
::data[format=table title="Infobox Galaxy"]
| Field | Value |
|---|---|
| name | NGC 3384 |
| image | Settling into old age NGC 3384.jpg |
| image_size | 250px |
| caption | NGC 3384 taken by Hubble. |
| constellation name | Leo{{cite book |
| editor | R. W. Sinnott |
| title | The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer |
| date | 1988 |
| publisher | Sky Publishing Corporation and Cambridge University Press |
| isbn | 978-0-933346-51-2}} |
| epoch | J2000 |
| type | E7{{cite web |
| title | NASA/IPAC Extragalactic Database |
| work | Results for NGC 3384 |
| url | http://nedwww.ipac.caltech.edu/ |
| access-date | 2006-10-12}} |
| ra | |
| dec | |
| dist_ly | 35.1 ± 2.3 Mly (10.8 ± 0.7 Mpc){{cite journal |
| author | Jensen, Joseph B. |
| title | Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations |
| journal | Astrophysical Journal |
| date | February 2003 |
| volume | 583 |
| issue | 2 |
| pages | 712–726 |
| bibcode | 2003ApJ...583..712J |
| doi | 10.1086/345430 |
| arxiv | astro-ph/0210129 |
| z | 704 ± 2 km/s |
| appmag_v | 10.9 |
| size_v | 5′.5 × 2′.5 |
| names | NGC 3371, UGC 5911, PGC 32292 |
| :: |
| name = NGC 3384 | image = Settling into old age NGC 3384.jpg | image_size = 250px | caption = NGC 3384 taken by Hubble. | constellation name = Leo{{cite book | editor=R. W. Sinnott | title= The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer | date=1988 | publisher=Sky Publishing Corporation and Cambridge University Press | isbn=978-0-933346-51-2}} | epoch = J2000 | type = E7{{cite web | title=NASA/IPAC Extragalactic Database | work=Results for NGC 3384 | url=http://nedwww.ipac.caltech.edu/ | access-date=2006-10-12}} | ra = | dec = | dist_ly = 35.1 ± 2.3 Mly (10.8 ± 0.7 Mpc){{cite journal | author=Jensen, Joseph B. | display-authors=4 | author2=Tonry, John L. | author3=Barris, Brian J. | author4=Thompson, Rodger I. | author5=Liu, Michael C. | author6=Rieke, Marcia J. | author7=Ajhar, Edward A. | author8=Blakeslee, John P. | title=Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations | journal=Astrophysical Journal |date=February 2003 | volume=583 | issue=2 | pages=712–726 | bibcode=2003ApJ...583..712J | doi=10.1086/345430 |arxiv = astro-ph/0210129 | s2cid=551714 }} | z = 704 ± 2 km/s | appmag_v = 10.9 | size_v = 5′.5 × 2′.5 | names = NGC 3371, UGC 5911, PGC 32292
NGC 3384 is an elliptical galaxy in the constellation Leo. The galaxy was discovered by William Herschel in 1784 as part of the Herschel 400 Catalogue. The high age of the stars in the central region of NGC 3384 was confirmed after analysis of their color. More than 80% were found to be Population II stars which are over a billion years old.{{cite journal | author=Attia, Abdel-Fattah | display-authors=4 | author2=Ismail, H. A. | author3=Selim, I. M. | author4=Osman, A. M. | author5=Isaa, I. A. | author6=Marie, M. A. | author7=Shaker, A. A. | title=Stellar Population Analysis of Galaxies based on Genetic Algorithms | journal=Chinese Journal of Astronomy and Astrophysics |date=August 2005 | volume=5 | issue=4 | pages=347–355 | bibcode=2005ChJAA...5..347A | doi=10.1088/1009-9271/5/4/002 | title=Populating the Galaxy Velocity Dispersion – Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values | last1=Graham | first1=Alister W. | postscript=. | journal=Publications of the Astronomical Society of Australia | volume=25 | issue=4 | pages=167–175 | date=November 2008 | doi=10.1071/AS08013 | bibcode=2008PASA...25..167G |arxiv = 0807.2549 | s2cid=89905 }}
Galaxy group information
::figure[src="https://upload.wikimedia.org/wikipedia/commons/f/f4/M105,NGC_3384&_NGC_3389.jpg" caption="M105]] (mid right), and [[NGC 3389]] (lower left)"] ::
NGC 3384 is a member of the M96 Group, a group of galaxies in the constellation Leo that is sometimes referred to as the Leo I Group. This group also includes the Messier objects M95, M96, and M105. All of these objects are conspicuously close to each other in the sky.{{cite book | author=R. B. Tully | date=1988 | title=Nearby Galaxies Catalog | publisher=Cambridge University Press | location=Cambridge | isbn=978-0-521-35299-4}}{{cite journal | author=P. Fouque | author2=E. Gourgoulhon | author3=P. Chamaraux | author4=G. Paturel | title=Groups of galaxies within 80 Mpc. II – The catalogue of groups and group members | journal=Astronomy and Astrophysics Supplement | date=1992 | volume=93 | pages=211–233 | bibcode=1992A&AS...93..211F}}{{cite journal | author=A. Garcia | title=General study of group membership. II – Determination of nearby groups | journal=Astronomy and Astrophysics Supplement | date=1993 | volume=100 | pages=47–90 | bibcode=1993A&AS..100...47G}}{{cite journal | author=G. Giuricin | author2=C. Marinoni | author3= L. Ceriani | author4= A. Pisani | title=Nearby Optical Galaxies: Selection of the Sample and Identification of Groups | journal=Astrophysical Journal | date=2000 | volume=543 | issue=1 | pages=178–194 | bibcode=2000ApJ...543..178G | doi=10.1086/317070|arxiv = astro-ph/0001140 | s2cid=9618325 }}
References
References
::callout[type=info title="Wikipedia Source"] This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page. ::