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Q248762

File:NGC_1232.jpg · Wikimedia Commons · See Wikimedia Commons

EntityQ248762· pop 39· linked from 494 articles

spiral galaxy in the constellation Eridanus

Key facts

Constellation
Eridanus
Right ascension
03 09 45.4322
Declination
−20 ° 34 ′ 44.443 ″
Heliocentric radial velocity
1603 ± 1 km/s
Distance
50.33 ± 2.84 Mly (15.432 ± 0.870 Mpc )
Type
SAB(rs)c
Size
145,300 ly (44.57 kpc ) (estimated)
Apparent size v
7′.4 × 6′.5
Notable features
Discrepant galaxy pair with NGC 1232 A

via Wikipedia infobox

Wikidata facts

Distance from Earth
23.4
Image
Spiral Galaxy NGC 1232.jpg
Show 9 more facts
galaxy morphological type
Sc
Commons category
NGC 1232
catalog code
LEDA 11819
time of discovery or invention
1784-10-20
apparent magnitude
7.381
radial velocity
1684
redshift
0.005347
right ascension
47.4396417
declination
-20.5793000
Sources (1)

via Wikidata · CC0

~6 min read

Article

NGC 1232, also known as the Eye of God Galaxy (not to be confused with the Helix Nebula, also known as Eye of God) is an intermediate spiral galaxy about 50 million light-years away in the constellation Eridanus. It was discovered by German-British astronomer William Herschel on 20 October 1784.

It is dominated by millions of bright stars and dark dust, in spiral arms rotating about the center. Open clusters containing bright blue stars are sprinkled along these spiral arms, with dark lanes of dense interstellar dust between. Less visible are dimmer stars and interstellar gas, comprising such a high mass that they dominate the dynamics of the inner galaxy. Not visible is matter of unknown form called dark matter, needed to explain the motions of the visible material in the outer galaxy. The galaxy is approximately 150,000 light-years across. The galaxy's spiral arms are not smooth and perturbed, leading to some suggesting a collision with a dwarf galaxy. However, some studies doubt this suggestion.

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