Scutum

For the Roman shield, see scutum (shield). For the zootomical term, see scute.
Scutum
Constellation

Abbreviation Sct
Genitive Scuti
Pronunciation /ˈskjuːtəm/,
genitive /ˈskjuːtaɪ/
Symbolism the Shield
Right ascension 18.7
Declination −10
Family Hercules
Quadrant SQ4
Area 109 sq. deg. (84th)
Main stars 2
Bayer/Flamsteed
stars		 7
Stars with planets 1
Stars brighter than 3.00m 0
Stars within 10.00 pc (32.62 ly) 0
Brightest star α Scuti (3.85m)
Nearest star LHS 3398
(41.54 ly, 12.74 pc)
Messier objects 2
Meteor showers June Scutids
Bordering
constellations		 Aquila
Sagittarius
Serpens Cauda
Visible at latitudes between +80° and −90°.
Best visible at 21:00 (9 p.m.) during the month of August.

Scutum is a small constellation introduced in the seventeenth century. Its name is Latin for shield.

History

The constellation Scutum as it can be seen by the naked eye.
Scutum Sobiescianum Firmamentum Sobiescianum sive Uranographia 1690
The shield of Sobieski - heraldry

Scutum was named in 1684 by Polish astronomer Johannes Hevelius[1] (Jan Heweliusz), who originally named it Scutum Sobiescianum (Shield of Sobieski) to commemorate the victory of the Christian forces led by Polish King John III Sobieski (Jan III Sobieski) in the Battle of Vienna in 1683. Later, the name was shortened to Scutum.

Five bright stars of Scutum (α Sct, β Sct, δ Sct, ε Sct and η Sct) were previously known as 1, 6, 2, 3, and 9 Aquilae respectively.[2]

Coincidentally, the Chinese also associated these stars with battle armor, incorporating them into the larger asterism known as Tien Pien, i.e., the Heavenly Casque (or Helmet).[3]

Notable features

Stars

Scutum is not a bright constellation, with the brightest star, Alpha Scuti, at magnitude 3.85. But some stars are notable in the constellation. Beta Scuti is the second brightest at magnitude 4.22, followed by Delta Scuti at magnitude 4.72. Beta Scuti is a binary system, with the primary with a spectral type similar to the Sun, although it is 1,270 times brighter. Delta Scuti is a bluish white giant star, which is now coming at the direction of the Solar System. Within 1.3 million years it will come as close to 10 light years from Earth, and will be much brighter than Sirius by that time.

Scutum is also notable for having UY Scuti, a red supergiant pulsating variable star. At 1,708 ± 192 solar radii, it is one of the largest stars currently known.

Deep sky objects

Although not a large constellation, Scutum contains several open clusters, as well as a globular cluster and a planetary nebula. The two best known deep sky objects in Scutum are M11 (the Wild Duck Cluster) and the open cluster M26 (NGC 6694). The globular cluster NGC 6712 and the planetary nebula IC 1295 can be found in the eastern part of the constellation, only 24 arcminutes apart.

The most prominent open cluster in Scutum is the Wild Duck Cluster, M11. It was named by William Henry Smyth in 1844 for its resemblance in the eyepiece to a flock of ducks in flight. The cluster, 6200 light-years from Earth and 20 light-years in diameter, contains approximately 3000 stars, making it a particularly rich cluster. It is 220 million years old.[4]

Space exploration

The Space probe Pioneer 11 is moving in the direction of this constellation, though it will not be nearing any of the stars in this constellation for many thousands of years, by which time its batteries will be long dead.

See also

Serpens held by Ophiuchus, as depicted in Urania's Mirror, a set of constellation cards published in London c. 1825. Above the tail of the serpent is the now-obsolete constellation Taurus Poniatovii while below it is Scutum.

References

  1. ↑ Star Tales ― Scutum by Ian Ridpath
  2. ↑ Wagman, M. (August 1987). "Flamsteed's Missing Stars". Journal for the History of Astronomy 18 (3): 212–213. Bibcode:1987JHA....18..209W.
  3. ↑ Richard H. Allen (1899) Star Names and Their Meanings, p. 363
  4. ↑ MacRobert, Alan (September 2012). "So, Where Are the Wild Ducks?!". Sky and Telescope.

External links

Wikimedia Commons has media related to Scutum.

Coordinates: 18h 42m 00s, −10° 00′ 00″

This article is issued from Wikipedia - version of the Tuesday, September 08, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.