NGC 4697

{{Short description|Elliptical galaxy in the constellation Virgo}}

{{Infobox Galaxy

| name = NGC 4697

| epoch = J2000

| constellation name = Virgo

| image = NGC_4697_HST_10003_R850_B475.png

| caption = NGC 4697 imaged by the Hubble Space Telescope

| type = E6{{cite web

| work=NASA/IPAC Extragalactic Database

| title=NED results for object NGC 4697

| url=http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+4697&extend=no

| access-date=2010-11-28 }}

| ra = {{RA|12|48|35.9}}

| dec = {{DEC|-05|48|03}}

| dist_ly = ~ 38 Mly / ~ 50 Mly{{cite simbad

| title=NGC 4697

| access-date=2010-11-28 }}

| z = 1241 ± 1 km/s

| size_v = 4.4{{prime}} × 2.8{{prime}}

| appmag_v = 10.97

| names = Caldwell 52, UGCA 300, MCG -01-33-010, PGC 043276

}}

NGC 4697 (also known as Caldwell 52) is an elliptical galaxy some 40 to 50 million light-years away in the constellation Virgo. It is a member of the NGC 4697 Group, a group of galaxies also containing NGC 4731 and several generally much smaller galaxies.{{cite web

| title=The Virgo II Groups

| work=Atlas of the Universe

| url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+4697

| access-date=2010-11-28 }} This group is about 55 million light-years away; it is one of the many Virgo II Groups, which form a southern extension of the Virgo Supercluster of galaxies.

The distance to NGC 4697 is not known with high precision: measurements vary from 28 to 76 million light-years. According to the NASA Extra-galactic Database, the average is about 38 million light-years; according to SIMBAD, about 50 million light-years.

The supermassive black hole at the core of NGC 4697 has a mass of {{Val|1.3e8|0.18|0.17|ul=solar mass}} as measured from Atacama Large Millimeter Array observations of the rotation of the central gas disk.{{cite journal |last1=Davis |first1=T. A. |last2=Bureau |first2=M. |last3=Onishi |first3=K. |last4=Cappellari |first4=M. |last5=Iguchi |first5=S. |last6=Sarzi |first6=M. |title=WISDOM Project - II. Molecular gas measurement of the supermassive black hole mass in NGC 4697 |journal=Monthly Notices of the Royal Astronomical Society |date=2017 |volume=468 |issue=4 |page=4675 |doi=10.1093/mnras/stw3217 |doi-access=free |bibcode=2017MNRAS.468.4675D|arxiv=1703.05248 }}

One supernova has been observed in NGC 4697: SN 2018imd (type Ia, mag. 15.5).[https://www.wis-tns.org/object/2018imd Transient Name Server entry for SN 2018imd.] Retrieved 23 March 2023.

On 2 April 1950, it was occulted by the Moon during a Total Lunar Eclipse over the Iberian Peninsula, Africa, Madagascar, Arabia and the Indian Ocean. This happened again under the same conditions on the April 1996 lunar eclipse over the same locations, and again during the April 2015 lunar eclipse over extreme NE Siberia and North America. It will next happen on 4 April 2080 over the Pacific Ocean including Hawaii.{{cite book |date=2002 |first=Jan |last=Meeus |chapter=Occultations of deep-sky objects during a total lunar eclipse |pages=157-162 |title=More Mathematical Astronomy Morsels |isbn=0943396743 |url=https://falakmu.id/khgt/dokumen/More%20mathematical%20astronomy%20morsels%20(Jean%20Meeus)%20(Z-Library).pdf}}{{rp|160}}