NGC 363

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NGC 363
NGC 363 DECam.jpg
DECam image of NGC 363
Observation data (J2000 epoch)
Constellation Cetus
Right ascension 01h 06m 15.8s [1]
Declination −16° 32 34 [1]
Redshift 0.037499 [1]
Helio radial velocity 11,242 km/s [1]
Distance 417 million ly (128 mpc) [1]
Apparent magnitude  (V)15.35 [1]
Characteristics
Type S0 [1]
Apparent size  (V)0.25' × 0.25' [1]
Other designations
MCG -03-03-023, 2MASX J01061580-1632343, 2MASXi J0106158-163233, 6dF J0106158-163234, PGC 3911. [1]

NGC 363 is a lenticular galaxy in the constellation Cetus. It was discovered on November 28, 1885 by Francis Leavenworth. It was described by Dreyer as "extremely faint, extremely small, round." [2]

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<span class="mw-page-title-main">NGC 350</span> Lenticular galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 351</span> Spiral galaxy in the constellation Cetus

NGC 351 is a spiral galaxy in the constellation Cetus. It was discovered on November 10, 1885 by Lewis Swift. It was described by Dreyer as "extremely faint, pretty small, northwestern of 2.", the other being NGC 353.

<span class="mw-page-title-main">NGC 353</span> Spiral galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 355</span> Galaxy in the constellation Cetus

NGC 355 is a lenticular galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "extremely faint, very small."

<span class="mw-page-title-main">NGC 359</span> Elliptical galaxy in the constellation Cetus

NGC 359 is an elliptical galaxy located approximately 238 million light-years from the Solar System in the constellation Cetus. It was discovered on September 2, 1864, by Albert Marth. It was described by Dreyer as "extremely faint, very small."

<span class="mw-page-title-main">NGC 360</span> Spiral galaxy in the constellation Tucana

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<span class="mw-page-title-main">NGC 389</span> Lenticular galaxy in constellation Andromeda

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<span class="mw-page-title-main">NGC 396</span> Lenticular galaxy in the constellation Pisces

NGC 396 is a lenticular galaxy located in the constellation Pisces. It was discovered on October 27, 1864 by Albert Marth. It was described by Dreyer as "extremely faint, small, a little extended."

<span class="mw-page-title-main">NGC 397</span> Lenticular galaxy in the constellation Pisces

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<span class="mw-page-title-main">NGC 409</span> Elliptical galaxy in the constellation of Sculptor

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<span class="mw-page-title-main">NGC 413</span> Spiral galaxy in the constellation Cetus

NGC 413 is a spiral galaxy of type SB(r)c located in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, pretty small, very little extended."

<span class="mw-page-title-main">NGC 417</span> Lenticular galaxy in the constellation Cetus

NGC 417 is a lenticular galaxy of type SAB0 located in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, extremely small, round."

<span class="mw-page-title-main">NGC 423</span> Lenticular galaxy in the constellation of Sculptor

NGC 423 is a lenticular galaxy of type S0/a? located in the constellation Sculptor. It was discovered on November 14, 1835 by John Herschel. It was described by Dreyer as "extremely faint, small, extended, gradually a little brighter middle, eastern of 2.", the other being NGC 418.

<span class="mw-page-title-main">NGC 435</span> Spiral galaxy in the constellation Cetus

NGC 435 is an intermediate spiral galaxy of type SAB(s)d: located in the constellation Cetus. It was discovered on October 23, 1864 by Albert Marth. It was described by Dreyer as "extremely faint, small, extended."

<span class="mw-page-title-main">NGC 5502</span> Galaxy within Ursa Major

NGC 5502 is a spiral galaxy in the constellation of Ursa Major, registered in New General Catalogue (NGC).

References

  1. 1 2 3 4 5 6 7 8 9 "NASA/IPAC Extragalactic Database". Results for NGC 0363. Retrieved September 2, 2016.
  2. "New General Catalog Objects: NGC 350 - 399". Cseligman. Retrieved November 25, 2016.