EntityQ1111603· pop 29· linked from 657 articles

NGC 4452

galaxy

In the Vinony graph

Within Vinony's link graph, NGC 4452 is referenced by 657 other articles, and connects out to list of stars in Virgo, NGC 4624 and list of NGC objects (4001–5000).

It is catalogued under topics including Astronomical objects discovered in 1784, Lenticular galaxies and NGC objects.

Its subject is documented across 29 Wikipedia language editions.

Key facts

Constellation: Virgo
Right ascension: 12 28.7 00
Declination: +11 ° 45 ′ 00 ″
Distance: 18.5 Mpc (60 Mly )
Group or cluster: Virgo
Type: S
Apparent size v: 2.7' × 36" (35 kly (11 kpc) in diameter)

via Wikipedia infobox

Wikidata facts

Instance of: lenticular galaxy
Constellation: Virgo
Distance from Earth: 18.95
Image: NGC 4452.jpg

Show 11 more facts

catalog code: Gaia DR2 3907556920868966528
right ascension: 187.18041002251450
Commons category: NGC 4452
discoverer or inventor: William Herschel
time of discovery or invention: 1784-03-15
apparent magnitude: 11.511
galaxy morphological type: S0
redshift: 0.000497
declination: 11.75505669959850
radial velocity: 162
epoch: J2000.0

Sources (1)

wikidata.org

via Wikidata · CC0

~1 min read

Encyclopedic overview

NGC 4452 is an edge-on lenticular galaxy that is part of the Virgo Cluster. NGC 4452 is about 60 million light-years (18 Mpc) away from Earth and 35 kly (11 kpc) in diameter. This galaxy was first seen by William Herschel in 1784 with his 47 cm (19 in) telescope.

NGC 4452 is so thin that it is actually difficult to determine what type of disk galaxy it is. Its lack of a visible dust lane indicates that it is a low-dust lenticular galaxy, although it is still possible that a view from on top would reveal spiral structure. The unusual stellar line segment spans about 35,000 light-years from end to end.

Excerpted from Wikipedia’s “NGC 4452” article, available under the CC BY-SA 4.0 licence.