NGC 6934 (also known as Caldwell 47) is a
globular cluster of stars in the northern
constellation
A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object.
The origins of the e ...
of
Delphinus
Delphinus (Pronounced or ) is a small constellation in the Northern Celestial Hemisphere, close to the celestial equator. Its name is the Latin
Latin (, or , ) is a classical language belonging to the Italic branch of the Indo-Europea ...
, about distant from the
Sun.
[ It was discovered by the German-born astronomer William Herschel on 24 September 1785.] The cluster is following a highly eccentric orbit (with an eccentricity of 0.81) through the Milky Way
The Milky Way is the galaxy that includes our Solar System, with the name describing the galaxy's appearance from Earth: a hazy band of light seen in the night sky formed from stars that cannot be individually distinguished by the naked eye ...
along an orbital plane that is inclined by 73° to the galactic plane. It may share a common dynamic origin with NGC 5466.[ As of 2018, it has been poorly studied.][
This appears to be a ]Oosterhoff type I
A globular cluster is a spheroidal conglomeration of stars. wikt:globular, Globular clusters are bound together by gravity, with a higher concentration of stars towards their centers. They can contain anywhere from tens of thousands to many mil ...
cluster with an intermediate metallicity
In astronomy, metallicity is the abundance of elements present in an object that are heavier than hydrogen and helium. Most of the normal physical matter in the Universe is either hydrogen or helium, and astronomers use the word ''"metals"'' as a ...
.[ It has an Shapley–Sawyer Concentration Class of VIII,][ with a ]core radius
A globular cluster is a spheroidal conglomeration of stars. Globular clusters are bound together by gravity, with a higher concentration of stars towards their centers. They can contain anywhere from tens of thousands to many millions of membe ...
of [ and a half-light radius of .][ The estimated mass is 295,000 times the ]mass of the Sun
The solar mass () is a standard unit of mass in astronomy, equal to approximately . It is often used to indicate the masses of other stars, as well as stellar clusters, nebulae, galaxies and black holes. It is approximately equal to the mass ...
.[ The cluster displays photometric anomalies, with a split subgiant branch on the ]HR diagram
HR, Hr or hr may refer to:
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* ''HR'', a 2013 television drama starring Alicia Silverstone
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.[ Searches for ]variable star
A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes with time. This variation may be caused by a change in emitted light or by something partly blocking the light, so variable stars are classified as ...
s have discovered 85 in the cluster field, of which 79 are of the RR Lyrae
RR Lyrae is a variable star in the Lyra constellation, figuring in its west near to Cygnus. As the brightest star in its class, it became the eponym for the RR Lyrae variable class of stars and it has been extensively studied by astro ...
class and one is a SX Phe variable.[ There is some evidence for a ]tidal tail
A tidal tail is a thin, elongated region of stars and interstellar gas that extends into space from a galaxy. Tidal tails occur as a result of galactic tide forces between interacting galaxies. Examples of galaxies with tidal tails include the ...
.[
]
References
External links
*
*
A Distant Backwater of the Milky Way
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/Hubble
The Hubble Space Telescope (often referred to as HST or Hubble) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the first space telescope, but it is one of the largest and most versa ...
Picture of the Week
{{DEFAULTSORT:NGC 6934
Globular clusters
Delphinus
6934
047b
Astronomical objects discovered in 1785