IC 592
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IC 592
Summary
IC 592 is a galaxy[1]. It has Wikipedia articles in 11 language editions, a strong signal of global cultural recognition.[2]
Key Facts
- IC 592's instance of is recorded as galaxy[3].
- IC 592's instance of is recorded as infrared source[4].
- IC 592's instance of is recorded as spiral galaxy[5].
- IC 592's constellation is recorded as Sextans[6].
- IC 592's galaxy morphological type is recorded as Sbc[7].
- IC 592's catalog code is recorded as IC 592[8].
- IC 592's catalog code is recorded as IRAS F10054-0215[9].
- IC 592's catalog code is recorded as UGC 5465[10].
- IC 592's catalog code is recorded as PGC 29465[11].
- IC 592's catalog code is recorded as MCG+00-26-020[12].
- IC 592's catalog code is recorded as GSC 04903-00824[13].
- IC 592's catalog code is recorded as 2dFGRS TGN217Z154[14].
- IC 592's catalog code is recorded as Z 8-45[15].
- IC 592's catalog code is recorded as 6dFGS gJ100758.8-022952[16].
- IC 592's catalog code is recorded as SDSS J100758.70-022951.8[17].
- IC 592's catalog code is recorded as UZC J100758.7-022953[18].
- IC 592's catalog code is recorded as Z 1005.4-0215[19].
- IC 592's catalog code is recorded as LEDA 29465[20].
- IC 592's catalog code is recorded as SDSS J101941.19+002700.6[21].
- IC 592's redshift is recorded as {'unit': '1', 'amount': '+0.020157'}[22].
- IC 592's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.0'}[23].
- IC 592's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+6055'}[24].
- IC 592's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+151.994792'}[25].
- IC 592's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-2.497806'}[26].
- IC 592's epoch is recorded as J2000.0[27].
Body
Definition and Type
Recorded instance of include galaxy[3], infrared source[4], and spiral galaxy[5].
Why It Matters
IC 592 has Wikipedia articles in 11 language editions, a strong signal of global cultural recognition.[2]