NGC 435

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NGC 435
NGC 0435 2MASS.jpg
NGC 435 as seen by 2MASS
Observation data (J2000 epoch)
Constellation Cetus
Right ascension 01h 13m 59.80s [1]
Declination +02° 04′ 15.00″ [1]
Redshift 0.03425±0.00004 [1]
Distance 478.4 Mly (146.68 Mpc) [1]
Apparent magnitude  (V)14.81 [1]
Characteristics
Type SAB(s)d:
Size196,000 ly[ citation needed ]
Apparent size  (V)1.122' x 0.437' [1]
Notable featuresN/A
Other designations
MCG+00-04-046, [1] PGC 4434, [1] UGC 779, [1] IRAS F01114+0148, [1] 2MASX J01135985+0204171, [1] Z 385-35, [1] UZC J011359.9+020416, [1] LEDA 4434 [1]

NGC 435 is an intermediate spiral galaxy located around 478 million light-years away in the constellation Cetus. [1] NGC 435 was discovered on October 23rd, 1864 by Albert Marth, and it does not have an active galactic nucleus or much star-formation. [1]

NGC 435 was described by John Louis Emil Dreyer as "extremely faint, small, extended."[ citation needed ]

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<span class="mw-page-title-main">NGC 4454</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 4464</span> Galaxy in the constellation of Virgo

NGC 4464 is an elliptical galaxy located about 70 million light-years away in the constellation of Virgo. NGC 4464 was discovered by astronomer William Herschel on December 28, 1785. NGC 4464 is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4623</span> Lenticular or elliptical galaxy in the constellation Virgo

NGC 4623 is an edge-on lenticular or elliptical galaxy located about 54 million light-years away in the constellation of Virgo. NGC 4623 is classified as an E7, a rare type of "late" elliptical that represents the first stage of transition into a lenticular galaxy. NGC 4623 was discovered by astronomer William Herschel on April 13, 1784. NGC 4623 is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4612</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 4919</span> Galaxy in the constellation Coma Berenices

NGC 4919 is a lenticular galaxy located about 340 million light-years away in the constellation of Coma Berenices. NGC 4919 was discovered by astronomer Heinrich d'Arrest on May 5, 1864. NGC 4919 is a member of the Coma Cluster.

<span class="mw-page-title-main">NGC 4907</span> Barred spiral galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4479</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4497</span> Lenticular galaxy in the constellation of Virgo

NGC 4497 is a lenticular galaxy located about 60 million light-years away in the constellation Virgo. NGC 4497 was discovered by astronomer William Herschel on March 15, 1784. It was rediscovered by astronomer Arnold Schwassmann on November 8, 1900 and was listed as IC 3452. NGC 4497 is a member of the Virgo Cluster.

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<span class="mw-page-title-main">NGC 4544</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 4578</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 4709</span> Galaxy in the constellation Centaurus

NGC 4709 is an elliptical galaxy located in the constellation Centaurus. It is considered to be a member of the Centaurus Cluster and is the dominant member of a small group of galaxies known as "Cen 45" which is currently merging with the main Centaurus Cluster even though the two subclusters' line of sight redshift velocities differ by about 1500 km/s. NGC 4709 was discovered by astronomer James Dunlop on May 7, 1826.

<span class="mw-page-title-main">NGC 4876</span> Galaxy in the constellation Coma Berenices

NGC 4876 is an elliptical galaxy located about 325 million light-years away in the constellation Coma Berenices. NGC 4876 was discovered by astronomer Guillaume Bigourdan on May 16, 1885. NGC 4876 is a member of the Coma Cluster.

<span class="mw-page-title-main">NGC 4892</span> Galaxy in the constellation Coma Berenices

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References

  1. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved February 27, 2024.


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