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EntityQ279134· pop 41· linked from 433 articles

Also known as Pavo Galaxy

spiral galaxy in the constellation Pavo

In the Vinony graph

Vinony's link graph records 433 inbound references to Q279134, and connects out to list of stars in Pavo, list of NGC objects (6001–7000) and Lagoon Nebula.

It is catalogued under topics including Astronomical objects discovered in 1826, Caldwell objects and Discoveries by James Dunlop.

Vinony links it to 41 Wikipedia language editions.

Key facts

Constellation
Pavo
Right ascension
19 09 46.1785
Declination
−63 ° 51 ′ 26.992 ″
Heliocentric radial velocity
841 ± 2 km/s
Distance
23.63 ± 1.68 Mly (7.244 ± 0.514 Mpc )
Group or cluster
Virgo Supercluster
Type
SAB(r)bc
Mass
5.92 × 10 M ☉
Size
~171,800 ly (52.68 kpc ) (estimated)
Apparent size v
20.0′ × 12.9′

via Wikipedia infobox

Wikidata facts

Distance from Earth
7
Image
Wide Field Imager view of a Milky Way look-alike NGC 6744.jpg
Show 9 more facts
time of discovery or invention
1826-06-30
galaxy morphological type
SAB(r)bc
Commons category
NGC 6744
catalog code
[VDD93] 223
redshift
0.002805
apparent magnitude
5.935
right ascension
287.4420792
declination
-63.8575389
radial velocity
833
Sources (1)

via Wikidata · CC0

~2 min read

Encyclopedic overview

NGC 6744 (also known as Caldwell 101 or the Pavo Galaxy) is an intermediate spiral galaxy in the constellation Pavo (Peacock). Its velocity with respect to the cosmic microwave background is 802 ± 3 km/s, which corresponds to a Hubble distance of 38.6 ± 2.7 Mly (11.82 ± 0.83 Mpc). However, 21 non redshift measurements give a distance of 23.63 ± 1.68 Mly (7.244 ± 0.514 Mpc). It was discovered on 30 June 1826 by Scottish astronomer James Dunlop, observing from Parramatta, Australia. It has a mass of 5.92×10 M☉.

One of the largest spiral galaxies in the local universe, NGC 6744 is considered a Milky Way mimic in the immediate vicinity, displaying remarkable star formation, flocculent (fluffy) arms, and an elongated core. It has at least one distorted companion galaxy (NGC 6744A) superficially similar to one of the Magellanic Clouds.

Excerpted from Wikipedia’s “Q279134” article, available under the CC BY-SA 4.0 licence.

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