IC 4537

Last updated
IC 4537
IC4537 - SDSS DR14.jpg
IC 4537 taken by SDSS
Observation data
Constellation Serpens
Right ascension 229.38 degrees
Declination 2.047 degrees
Redshift 0.05424 0.00001
Heliocentric radial velocity 16,262 km/s
Distance 736 Mly (225.6 Mpc)
Apparent magnitude  (V)12.605
Surface brightness 23.9 mag/arcsec
Characteristics
Type E3, LINER
Other designations
PGC 54583, CGCG 021-070, 2MASX J15173246+0202504, SDSS J151732.44+020250.6, NSA 125157, ASK 695467.0, LEDA 54583

IC 4537 is a type S0-a [1] lenticular galaxy located in the Serpens constellation. [2] It is located 736 million light-years from the Solar System [3] and was found by astronomer Edward Emerson Barnard [4] although the year of discovery was unknown. IC 4537 has a surface brightness of magnitude 23.9 and a right ascension of (15 hours: 17.5 minutes) and declination (+0.2 degrees : 02 minutes). [5] IC 4537 is apparently located a few miles away from the globular cluster, Messier 5. [6]

Related Research Articles

<span class="mw-page-title-main">NGC 3285</span> Galaxy in the constellation Hydra

NGC 3285 is a barred spiral galaxy located about 200 million light-years away in the constellation Hydra. The galaxy was discovered by astronomer John Herschel on March 24, 1835. NGC 3285 is a member of the Hydra Cluster.

<span class="mw-page-title-main">IC 3971</span> Spiral galaxy located in the constellation Coma Berenices

IC 3971 is a spiral galaxy located approximately 1 billion light-years away from the Solar System, in the constellation of Coma Berenices. It was first discovered in January 1904 by German astronomer Max Wolf. According to SIMBAD database, it is a LINER type galaxy with an active nucleus.

<span class="mw-page-title-main">IC 64</span> Galaxy in the constellation Pisces

IC 64 is a massive lenticular galaxy located 622 million light-years away in the Pisces constellation. IC 64 has a diameter of 300,000 thousand light-years, making it, three times bigger than the Milky Way and one of the largest galaxies observed. IC 64 was discovered by Stephane Javelle, a French astronomer on 5th December, 1893. It has an active galactic nucleus and is considered a radio galaxy.

<span class="mw-page-title-main">IC 3053</span> Galaxy in the constellation Coma Berenices

IC 3053 is a type Sab barred spiral galaxy with a ring located in the Coma Berenices constellation. The galaxy lies 720 million light-years from the solar system and has an estimated diameter of 180,000 light-years meaning the galaxy is much larger compared to the Milky Way. IC 3053 was first discovered by Royal Harwood Frost on May 7, 1904. Despite listed in the Virgo Cluster Catalogue as VCC 95, it is not a member of the Virgo Cluster due to its high redshift and instead a background galaxy.

<span class="mw-page-title-main">IC 3031</span> Galaxy in the constellation Coma Berenices

IC 3031 known as PGC 92941, is an edge-on spiral galaxy located in the Coma Berenices constellation. The galaxy lies 1.15 billion light-years away from the Solar System and has an estimated diameter of 240,000 light-years meaning it is bigger compared to the Milky Way. IC 3031 was discovered by astronomer Royal Harwood Frost on May 7, 1904.

<span class="mw-page-title-main">IC 3246</span> Galaxy in the constellation Virgo

IC 3246 known as PGC 40202, is a barred spiral galaxy with a ring located in the Virgo constellation. It is situated 1.13 billion light-years away from the Solar System and was discovered by Friedrich Karl Arnold Schwassmann on September 14, 1900. IC 3246 has a surface brightness of 23.6 magnitude/arc seconds and located at right ascension and declination respectively.

<span class="mw-page-title-main">IC 2800</span> Galaxy in the constellation Leo

IC 2800 known as PGC 3543021, is a late type spiral galaxy located 750 million light-years away from the Milky Way in the Leo constellation. It has a diameter of 110,000 light-years and was discovered on March 27, 1906, by German astronomer, Max Wolf. It has a surface brightness of magnitude 24.0 and is located at right ascension (11:24:27:08) and declination (12:12:31.70).

<span class="mw-page-title-main">IC 3482</span> Galaxy in the constellation Coma Berenices

IC 3482 is a type Sb spiral galaxy in the Coma Berenices constellation. It is located 850 million light-years away from the Solar System. IC 3482 has an apparent size of 0.4 x 0.15 arcmin, meaning it has estimated diameter of 140,000 light-years. IC 3482 was discovered on March 23, 1903, by German astronomer pioneer, Max Wolf. It is located at right ascension of (12:33:01.00) and declination of (27:49:49:10), and has a surface brightness of magnitude 23.

<span class="mw-page-title-main">IC 3786</span> Galaxy in the constellation Canes Venatici

IC 3786 is a type Sbc spiral galaxy in the Canes Venatici constellation. It is located 755 million light-years from the Milky Way and was discovered by Max Wolf on March 21, 1903.

<span class="mw-page-title-main">IC 3789</span> Galaxy in the constellation Coma Berenices

IC 3789, occasionally known as PGC 1619535, is a type Sbc barred spiral galaxy in the Coma Berenices constellation. It is located 872 million light-years away from the Solar System and has an approximate diameter of 150,000 light-years making it slightly larger than the Milky Way. IC 3789 was discovered on 27 January 1904 by astronomer Max Wolf.

<span class="mw-page-title-main">IC 4000</span> Galaxy in the constellation Canes Venatici

IC 4000 known as PGC 2152407, is a type Sbc spiral galaxy with a ring in the constellation of Canes Venatici. It is located 1.5 billion light-years away from the solar system and has an estimated diameter of 100,000 light-years which is the same length as the Milky Way. IC 4000 was discovered by Max Wolf on March 21, 1903. It has a surface brightness of 23.3 magnitude/arc seconds and located right ascension (12:59:36.62) and declination (39:35:15:90).

<span class="mw-page-title-main">IC 4026</span> Galaxy in the constellation Coma Berenices

IC 4026 is a type S0 lenticular galaxy with a bar located in Coma Berenices. It is located 315 million light-years away from the Solar System and has an approximate diameter of 70,000 light-years which is less the size of the Milky Way. IC 4026 was discovered on May 11, 1896, by astronomer Hermann Kobold and is a member of the Coma Cluster. It has a surface brightness of 11.99 mag/arcsecs meaning it is a high surface brightness galaxy.

<span class="mw-page-title-main">IC 2628</span> Galaxy in the constellation Leo

IC 2628 is a type SBa barred spiral galaxy with a ring located in Leo constellation. It is located 600 million light-years from the Solar System and has an approximate diameter of 135,000 light-years. IC 2628 was discovered on March 27, 1906, by Max Wolf and is classified as a ring galaxy due to its peculiar appearance. The galaxy has a surface brightness of magnitude 23.8 and located at right ascension (11:11:37.8) and declination (+12:07:21) respectively.

<span class="mw-page-title-main">IC 535</span> Galaxy in the constellation Hydra

IC 535 known as PGC 26524 and PGC 1128295, is a type E elliptical galaxy with a ring located in the Hydra constellation. It is located 740 million light-years away from the Solar System and has an estimated diameter of 85,000 light-years. IC 535 was discovered on March 23, 1893, by Stephane Javelle. It has a surface brightness of 23.7 mag/arcsec and is moving at radial velocity of 16,049 kilometers per seconds. It is located at right ascension and declination.

<span class="mw-page-title-main">IC 2431</span> Interacting galaxies in the constellation Cancer

IC 2431 are a group of interacting galaxies in the constellation of Cancer. They are located 684 million light-years away from the Solar System and were discovered on February 24, 1896, by Stephane Javelle.

<span class="mw-page-title-main">IC 1166</span> Pair of galaxies in Corona Borealis

IC 1166 are a pair of galaxies in the Corona Borealis constellation comprising IC 1166 NED01 and IC 1166 NED02. They are located 977 million light-years from the Solar System and were discovered on July 28, 1892, by Stephane Javelle.

<span class="mw-page-title-main">IC 1185</span> Spiral galaxy located in Hercules

IC 1185 is a type Sab spiral galaxy located in Hercules. It is located 420 million light-years from the Solar System and has an approximate diameter of 115,000 light-years. IC 1185 was discovered on June 8, 1888, by astronomer Guillaume Bigourdan and is a member of the Hercules Cluster. IC 1185 has a surface brightness of magnitude 22.7 and presents a double nucleus, which might represent a late stage of galaxy merger.

<span class="mw-page-title-main">IC 2759</span> Elliptical galaxy in the constellation of Leo

IC 2759 is a small type E elliptical galaxy located in the constellation of Leo. It is located 350 million light-years away from the Solar System and was discovered on April 24, 1897, by Guillaume Bigourdan. Sometimes IC 2759 is confused with the spiral galaxy, PGC 34882 which is located south of the galaxy.

<span class="mw-page-title-main">IC 2816</span>

IC 2816 known as PGC 3472124, is a type Sbc spiral galaxy with a ring structure located in the Leo constellation. It is located 878 million light-years from the Solar System and has apparent dimensions of 0.59 x 0.22 arcmin, meaning its diameter is 160,000 light-years across.

IC 4588 is a type E elliptical galaxy located in the constellation Serpens. It is located 729 million light-years from the Solar System and has a dimension of 0.30 x 0.3 arcmin meaning its diameter is 64,000 light-years across. IC 4588 was discovered by Stephane Javelle on July 15, 1903.

References

  1. "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-04-28.
  2. Astronomy, Go. "IC 4537 | galaxy in Serpens | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-04-28.
  3. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-28.
  4. "Index Catalog Objects: IC 4500 - 4549". cseligman.com. Retrieved 2024-04-28.
  5. "IC 4537". spider.seds.org. Retrieved 2024-04-28.
  6. Pommier, Rod. "M5 AND GALAXY IC 4537 IN SERPENS". Sky & Telescope. Retrieved 2024-04-28.