Messier 32 (M32), also known as Le Gentil, is a dwarf elliptical galaxy located in Andromeda constellation.
The galaxy lies at a distance of 2.49 million light years from Earth and has an apparent magnitude of 8.08. M32 is a satellite galaxy of M31, the famous Andromeda Galaxy. It has the designation NGC 221 in the New General Catalogue.
Messier 32 was named after Guillaume Le Gentil, the French astronomer who discovered it in 1749. The dwarf galaxy spans only 6,500 light years at its widest point and occupies an area 8.7 by 6.5 arc minutes in size in the sky.
Le Gentil can be seen in binoculars and appears like a hazy patch of light. In small telescopes, it looks like a diffuse ball of light with a bright core, surrounded by a small halo.
8-inch telescopes will reveal the galaxy’s oval shape, but even larger instruments will not show much detail because M32 is very small, especially when compared to M31.
Messier 32 is a member of the Local Group of galaxies, which also includes the Andromeda Galaxy (M31), the Triangulum Galaxy (M33) and the Milky Way among others. It was the first elliptical galaxy to be discovered.
Messier 32 is easy to find as it appears right next to the Andromeda Galaxy. It can be found by first locating the Great Square of Pegasus, formed by three stars that belong to Pegasus constellation (Scheat, Markab and Algenib) and Alpheratz, Alpha Andromedae. Alpheratz marks the northeastern corner of the square, the one facing Cassiopeia‘s famous W shape. With an apparent magnitude of 2.1, it is the brightest of the four stars.
Going northeast of Alpheratz and looking under the W asterism, the three bright stars of Andromeda constellation are easy to spot: Delta Andromedae lies about 7 degrees from Alpheratz, Mirach (Beta Andromedae) is a further 8 degrees away, and Almach (Gamma Andromedae) is the third bright star along the same line and the closest one to Cassiopeia.
The Andromeda Galaxy and Le Gentil can be found 8 degrees to the northwest of the middle star, Mirach. Le Gentil lies 22 arc minutes south of Andromeda‘s centre. It appears superimposed on Andromeda‘s outer spiral arm and is believed to be closer to us than that particular portion of the larger galaxy. (Even though Andromeda is usually listed as some 110,000 light years more distant than M32, it is still uncertain which of the two galaxies is closer to us.) The best time of year to observe M32 from northern latitudes is in the months of October, November and December.
Le Gentil contains almost no gas or dust and shows no evidence of any current star forming activity, but there are indications that star formation took place in the galaxy in the past. Like other elliptical galaxies, M32 is home to mostly old red and yellow stars.
Messier 32 has a linear diameter of 6,550 by 5,000 light years and a total mass of about 3 billion solar masses. It is approaching us at 205 km/s. The galaxy’s overall spectral class is G3.
The galaxy contains a supermassive black hole at its centre. The mass of the black hole is estimated to be in the range from 1.5 and 5 million solar masses.
Messier 32 is one of Andromeda Galaxy‘s 14 known satellite galaxies and one of the two brightest ones. The other bright dwarf elliptical galaxy, Messier 110, is more distant. Both galaxies were first resolved by the German astronomer Walter Baade in 1944. Baade used the 100-inch telescope at the Mount Wilson Observatory in Los Angeles.
Messier 32 is a prototype for a class of galaxies known as compact ellipticals. It is believed to have once been a spiral galaxy, but as a result of interaction with the much larger Andromeda, its spiral arms were ripped off by the tidal forces from M31 and its stars and globular clusters now reside in the larger galaxy’s halo.
American astronomer Halton Arp included Le Gentil in his Atlas of Peculiar Galaxies (1966) as Arp 168. M32 is listed in the category of galaxies with diffuse counter-tails (tidal features caused by gravitational interactions with another galaxy).
A nova was detected in M32 on August 31, 1998. It occurred about 28.5 arc seconds west and 44.7 arc seconds south of the galaxy’s centre and was discovered by a team of astronomers from the University of California at Berkeley, within the Lick Observatory Supernova Search Program. The nova reached a visual magnitude of 16.5.
Guillaume Le Gentil discovered the galaxy on October 29, 1749. He noted, “While observing the Andromeda Nebula with a fine 18-foot telescope … I saw another small nebula, about one minute in diameter which appeared to throw out two small rays; one to the right and the other to the left.“
Charles Messier first observed the galaxy in 1757 and catalogued it on August 3, 1764, also thinking that it was a nebula. Messier wrote:
I have examined in the same night [August 3 to 4, 1764], & with the same instruments, the small nebula which is below & at some [arc] minutes from that in the girdle of Andromeda [Messier 31]. M. le Gentil discovered it on October 29, 1749. I saw it for the first time in 1757. When I examined the former, I did not know previously of the discovery which had been made by M. Le Gentil, although he had published it in the second volume of the Memoires de Savans érangers, page 137. Here is what I found written in my journal of 1764. That small nebula is round & may have a diameter of 2 minutes of arc: between that small nebula & that in the girdle of Andromeda one sees two small telescopic stars. In 1757, I made a drawing of that nebula, together with the old one, & I have not found and change at each time I have reviewed it: One sees with difficulty that nebula with an ordinary [non-achromatic] refractor of three feet & a half; its light is fainter than that of the old one, & it doesn’t contain any star. At the passage of that new nebula through the Meridian, comparing it with the star Gamma Andromedae, I have determined its position in right ascension as 7d 27′ 32″, & its declination as 38d 45′ 34″ north.
William Herschel observed M32 in 1785 and described it as a “pretty large round nebula, much condensed in the middle, and south following the great one.“
John Herschel catalogued M32 as h 51 in 1828, observing that it is a “companion of the great nebula. Extremely bright; pretty large; there is a brighter middle to a star of 10 mag; 40″ diameter.“
|Type: Dwarf elliptical|
|Designations: Messier 32, M32, Le Gentil, NGC 221, Arp 168, PGC 2555, UGC 452, LEDA 2555, BD+40 147, IRAS 00399+4035|
|Features: Satellite galaxy of M31|
|Right ascension: 00h 42m 41.8s|
|Declination: +40°51’55” vv|
|Distance: 2.49 million light years (763,000 parsecs)|
|Apparent magnitude: 8.08|
|Apparent dimensions: 8′.7 x 6′.5|
|Radius: 3,275×2,500 light years|
|Redshift: -200 km/s|