Sculptor (constellation)

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Sculptor
Constellation
Sculptor IAU.svg
List of stars in Sculptor
AbbreviationScl
Genitive Sculptoris
Pronunciation /ˈskʌlptər/ ,
genitive /skəlpˈtɒrɪs/
Symbolismthe Sculptor
Right ascension 0h
Declination −30°
QuadrantSQ1
Area 475 sq. deg. (36th)
Main stars 4
Bayer/Flamsteed
stars		18
Stars with planets 6
Stars brighter than 3.00m0
Stars within 10.00 pc (32.62 ly)2
Brightest star α Scl  (4.30 m )
Messier objects 0
Bordering
constellations		 Cetus
Aquarius
Piscis Austrinus
Grus
Phoenix
Fornax
Visible at latitudes between +50° and −90°.
Best visible at 21:00 (9 p.m.) during the month of November.

Sculptor is a faint constellation in the southern sky. It represents a sculptor. It was introduced by Nicolas Louis de Lacaille in the 18th century. He originally named it Apparatus Sculptoris (the sculptor's studio), but the name was later shortened.

Contents

History

Artistic rendition of the sculptor's studio, along with parts of the neighbouring constellations of Cetus and Machina Electrica, in Urania's Mirror (1825) Sculptor-Sydney-Hall.jpg
Artistic rendition of the sculptor's studio, along with parts of the neighbouring constellations of Cetus and Machina Electrica, in Urania's Mirror (1825)

The region to the south of Cetus and Aquarius had been named by Aratus in 270 BC as The Waters – an area of scattered faint stars with two brighter stars standing out. Professor of astronomy Bradley Schaefer has proposed that these stars were most likely Alpha and Delta Sculptoris. [1]

The French astronomer Nicolas-Louis de Lacaille first described the constellation in French as l'Atelier du Sculpteur (the sculptor's studio) in 1751–52, [2] [3] depicting a three-legged table with a carved head on it, and an artist's mallet and two chisels on a block of marble alongside it. [4] Lacaille had observed and catalogued almost 10,000 southern stars during a two-year stay at the Cape of Good Hope, devising fourteen new constellations in uncharted regions of the Southern Celestial Hemisphere not visible from Europe. He named all but one in honour of instruments that symbolised the Age of Enlightenment. [lower-alpha 1] [5]

Characteristics

The constellation of Sculptor can be seen with the naked eye. Constellation Sculptor.jpg
The constellation of Sculptor can be seen with the naked eye.

Sculptor is a small constellation bordered by Aquarius and Cetus to the north, Fornax to the east, Phoenix to the south, Grus to the southwest, and Piscis Austrinus to the west. The bright star Fomalhaut is nearby. [6] The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is "Scl". [7] The official constellation boundaries, as set by Belgian astronomer Eugène Delporte in 1930, [lower-alpha 2] are defined by a polygon of 6 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 23h 06.4m and 01h 45.5m, while the declination coordinates are between −24.80° and −39.37°. [9] The whole constellation is visible to observers south of latitude 50°N. [lower-alpha 3]

In the constellation Sculptor lies this large extended spiral galaxy called NGC 289. Despite being around 75 million light-years away, the light of NGC 289 is stunningly captured here by the Dark Energy Camera (DECam). Gentle Giant Galaxy (iotw2332a).jpg
In the constellation Sculptor lies this large extended spiral galaxy called NGC 289. Despite being around 75 million light-years away, the light of NGC 289 is stunningly captured here by the Dark Energy Camera (DECam).

Notable features

Stars

Curious spiral around red giant star R Sculptoris Curious spiral spotted by ALMA around red giant star R Sculptoris (data visualisation).jpg
Curious spiral around red giant star R Sculptoris

No stars brighter than 3rd magnitude are located in Sculptor. This is explained by the fact that Sculptor contains the south galactic pole [12] where stellar density is very low.[ citation needed ] Overall, there are 56 stars within the constellation's borders brighter than or equal to apparent magnitude 6.5. [lower-alpha 4] [10]

The brightest star is Alpha Sculptoris, an SX Arietis-type variable star with a spectral type B7IIIp and an apparent magnitude of 4.3. [14] It is 780 ± 30 light-years distant from Earth. [15]

Eta Sculptoris is a red giant of spectral type M4III that varies between magnitudes 4.8 and 4.9, pulsating with multiple periods of 22.7, 23.5, 24.6, 47.3, 128.7 and 158.7 days. [16] Estimated to be around 1,082 times as luminous as the Sun, [17] it is 460 ± 20 light-years distant from Earth. [18]

R Sculptoris is a red giant that has been found to be surrounded by spirals of matter likely ejected around 1800 years ago. It is 1,440 ± 90 light-years distant from Earth. [19]

The Astronomical Society of Southern Africa in 2003 reported that observations of the Mira variable stars T, U, V and X Sculptoris were very urgently needed as data on their light curves was incomplete. [20]

Deep sky objects

The constellation also contains the Sculptor Dwarf, a dwarf galaxy which is a member of the Local Group, as well as the Sculptor Group, the group of galaxies closest to the Local Group. The Sculptor Galaxy (NGC 253), a barred spiral galaxy and the largest member of the group, lies near the border between Sculptor and Cetus. Another prominent member of the group is the irregular galaxy NGC 55.

One unique galaxy in Sculptor is the Cartwheel Galaxy, at a distance of 500 million light-years. The result of a merger around 300 million years ago, the Cartwheel Galaxy has a core of older, yellow stars, and an outer ring of younger, blue stars, which has a diameter of 100,000 light-years. The smaller galaxy in the collision is now incorporated into the core, after moving from a distance of 250,000 light-years. The shock waves from the collision sparked extensive star formation in the outer ring. [21]

Namesakes

Sculptor (AK-103) was a United States Navy Crater class cargo ship named after the constellation.

See also

Related Research Articles

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<span class="mw-page-title-main">Pi Sculptoris</span> Star in the constellation Sculptor

π Sculptoris, Latinized as Pi Sculptoris, is candidate astrometric binary star system in the southern constellation Sculptor, positioned near the eastern constellation border with Fornax. It has an orange hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.25. Based upon parallax measurements, the system is located at a distance of 66 light years from the Sun, and is drifting further away with a radial velocity of +14 km/s.

Kappa2 Sculptoris, Latinized from κ2 Sculptoris, is a solitary, orange-hued star in the southern constellation of Sculptor. It is faintly visible to the naked eye, with a combined apparent visual magnitude of +5.42. Based upon an annual parallax shift of 4.11 mas as measured from Earth, it is located approximately 800 light years from the Sun.

<span class="mw-page-title-main">H Scorpii</span> Star in the constellation Scorpius

H Scorpii is a single star in the southern constellation Scorpius. It is faintly visible to the naked eye with an apparent visual magnitude of 4.18. The star is located at a distance of approximately 343 light-years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −2 km/s. This star was initially given the Bayer designation Beta Normae by Lacaille but it was later reassigned from Norma to Scorpius.

References

Notes

  1. ↑ The exception is Mensa, named for the Table Mountain. The other thirteen (alongside Sculptor) are Antlia, Caelum, Circinus, Fornax, Horologium, Microscopium, Norma, Octans, Pictor, Pyxis, Reticulum and Telescopium. [5]
  2. ↑ Delporte had proposed standardising the constellation boundaries to the International Astronomical Union, who had agreed and gave him the lead role [8]
  3. ↑ While parts of the constellation technically rise above the horizon to observers between 50°N and 65°N, stars within a few degrees of the horizon are to all intents and purposes unobservable. [10]
  4. ↑ Objects of magnitude 6.5 are among the faintest visible to the unaided eye in suburban-rural transition night skies. [13]

Citations

  1. ↑ Schaefer, Bradley E. (2002). "The latitude and epoch for the formation of the southern Greek constellations". Journal for the History of Astronomy. 33, part 4 (113): 313–50. Bibcode:2002JHA....33..313S. doi:10.1177/002182860203300401. ISSN   0021-8286. S2CID   122459258.
  2. ↑ Ridpath, Ian. "Lacaille's Southern Planisphere of 1756". Star Tales. Self-published. Retrieved 25 August 2015.
  3. ↑ Lacaille, Nicolas Louis (1756). "Relation abrégée du Voyage fait par ordre du Roi au cap de Bonne-espérance". Mémoires de l'Académie Royale des Sciences (in French): 519–592 [589].
  4. ↑ Ridpath, Ian. "Sculptor". Star Tales. Retrieved 3 December 2016.
  5. 1 2 Wagman 2003, pp. 5–6.
  6. ↑ Klepešta, Josef; Rükl, Antonín (1974) [1969]. Constellations. Hamlyn. pp.  234–35. ISBN   0-600-00893-2.
  7. ↑ Russell, Henry Norris (1922). "The new international symbols for the constellations". Popular Astronomy. 30: 469. Bibcode:1922PA.....30..469R.
  8. ↑ Ridpath, Ian. "Constellation boundaries: How the modern constellation outlines came to be". Star Tales. self-published. Retrieved 1 June 2016.
  9. ↑ "The Constellations: Sculptor, constellation boundary". International Astronomical Union . Retrieved 4 December 2016.
  10. 1 2 Ridpath, Ian. "Constellations". Star Tales. self-published. Retrieved 1 June 2016.
  11. ↑ "Surprising Spiral Structure Spotted by ALMA". ESO Press Release. Retrieved 11 October 2012.
  12. ↑ Blaauw, A.; Gum, C.S.; Pawsey, J.L.; Westerhout, G. (1960). "The new IAU system of galactic coordinates (1958 revision)". Monthly Notices of the Royal Astronomical Society . 121 (2): 123. Bibcode:1960MNRAS.121..123B. doi: 10.1093/mnras/121.2.123 .
  13. ↑ Bortle, John E. (February 2001). "The Bortle Dark-Sky Scale". Sky & Telescope . Sky Publishing Corporation. Retrieved 4 March 2016.
  14. ↑ "Alpha Sculptoris– Rotationally Variable Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 5 December 2013.
  15. ↑ van Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv: 0708.1752 . Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID   18759600.
  16. ↑ Tabur, V.; Bedding, T. R. (2009). "Long-term photometry and periods for 261 nearby pulsating M giants". Monthly Notices of the Royal Astronomical Society . 400 (4): 1945–61. arXiv: 0908.3228 . Bibcode:2009MNRAS.400.1945T. doi:10.1111/j.1365-2966.2009.15588.x. S2CID   15358380.
  17. ↑ McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental parameters and infrared excesses of Hipparcos stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–357. arXiv: 1208.2037 . Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x. S2CID   118665352. Vizier catalog entry
  18. ↑ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics . 616. A1. arXiv: 1804.09365 . Bibcode: 2018A&A...616A...1G . doi: 10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
  19. ↑ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics . 616. A1. arXiv: 1804.09365 . Bibcode: 2018A&A...616A...1G . doi: 10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
  20. ↑ Cooper, Tim (2003). "Presidential address: Amateur Observations – Successes and Opportunities". Monthly Notes of the Astronomical Society of Southern Africa. 62: 234–240. Bibcode:2003MNSSA..62..234C.
  21. ↑ Wilkins, Jamie; Dunn, Robert (2006). 300 Astronomical Objects: A Visual Reference to the Universe. Buffalo, New York: Firefly Books. ISBN   978-1-55407-175-3.

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