NGC 3532

Last updated
NGC 3532
Eso1439a.jpg
Observation data (J2000 epoch)
Right ascension 11h 05m 33s [1]
Declination −58° 43.8 [1]
Distance 1,321 [2] ly (405 pc)
Physical characteristics
Other designations NGC 3532, [1] Caldwell 91, Cr 238, Mel 103, C 1104-584, Cl* 1104-584, CL 1104-584, Lacaille II.10, [3] Football Cluster, Wishing Well Cluster [4] [5] [6] [7]
Associations
Constellation Carina
See also: Open cluster, List of open clusters

NGC 3532 (Caldwell 91), [8] also commonly known as the Pincushion Cluster, [9] [10] [11] [8] Football Cluster, [12] [13] the Black Arrow Cluster, [14] or the Wishing Well Cluster, [4] [5] [6] [7] is an open cluster some 405 parsecs from Earth [2] in the constellation Carina. Its population of approximately 150 stars of 7th magnitude or fainter includes seven red giants [15] and seven white dwarfs. [16] [17] On 20 May 1990 it became the first target ever observed by the Hubble Space Telescope. A line from Beta Crucis through Delta Crucis passes somewhat to the north of NGC 3532. The cluster lies between the constellation Crux and the larger but fainter "False Cross" asterism. The 4th-magnitude Cepheid variable star x Carinae (V382 Car) appears near the southeast fringes, but it lies between the Sun and the cluster and is not a member of the cluster.

Contents

The cluster was first catalogued by Nicolas Louis de Lacaille in 1752. [18] It was admired by John Herschel, who thought it one of the finest star clusters in the sky, [3] [19] with many double stars (binary stars). [20]

Hubble first light

This is the first light image for the Wide Field and Planetary Camera of the Hubble Space Telescope, taken in May 1990; this view is near star HD96755 in the open cluster NGC 3532. This view is 11 by 14 arcseconds of the sky. Hubble First Light, First Released Image (STScI-1990-04a).png
This is the first light image for the Wide Field and Planetary Camera of the Hubble Space Telescope, taken in May 1990; this view is near star HD96755 in the open cluster NGC 3532. This view is 11 by 14 arcseconds of the sky.
This New Horizons image, taken with the LORRI instrument and captured on December 5, 2017, broke the record for an image taken at the greatest distance from Earth, surpassing Pale Blue Dot taken by Voyager 1. Wishing Well cluster New Horizons.png
This New Horizons image, taken with the LORRI instrument and captured on December 5, 2017, broke the record for an image taken at the greatest distance from Earth, surpassing Pale Blue Dot taken by Voyager 1.

Related Research Articles

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<span class="mw-page-title-main">Fornax</span> Constellation in the southern celestial hemisphere

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<span class="mw-page-title-main">Hydrus</span> Constellation in the southern celestial hemisphere

Hydrus is a small constellation in the deep southern sky. It was one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm (14 in) diameter celestial globe published in late 1597 in Amsterdam by Plancius and Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer's Uranometria of 1603. The French explorer and astronomer Nicolas Louis de Lacaille charted the brighter stars and gave their Bayer designations in 1756. Its name means "male water snake", as opposed to Hydra, a much larger constellation that represents a female water snake. It remains below the horizon for most Northern Hemisphere observers.

<span class="mw-page-title-main">Microscopium</span> Minor constellation in the southern celestial hemisphere

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<span class="mw-page-title-main">Pyxis</span> Constellation in the southern celestial hemisphere

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<span class="mw-page-title-main">Circinus</span> Constellation in the southern celestial hemisphere

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<span class="mw-page-title-main">Messier 4</span> Globular cluster in Scorpius

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<span class="mw-page-title-main">NGC 6397</span> Globular cluster of stars in the Milky Way

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<span class="mw-page-title-main">Jewel Box (star cluster)</span> Open cluster in the constellation Crux

The Jewel Box is an open cluster in the constellation Crux, originally discovered by Nicolas Louis de Lacaille in 1751–1752. This cluster was later named the Jewel Box by John Herschel when he described its telescopic appearance as "...a superb piece of fancy jewellery". It is easily visible to the naked eye as a hazy star some 1.0° southeast of the first-magnitude star Mimosa. This hazy star was given the Bayer star designation "Kappa Crucis", from which the cluster takes one of its common names. The modern designation Kappa Crucis has been assigned to one of the stars in the base of the A-shaped asterism of the cluster

<span class="mw-page-title-main">Butterfly Cluster</span> Open cluster in Scorpius

The Butterfly Cluster is an open cluster of stars in the southern constellation of Scorpius. Its name derives from the vague resemblance of its shape to a butterfly. The Trumpler classification of II 3 r encodes it is rich in stars, ranks II out of IV for disparateness and greatly mixes bright with faint components. It is 3.5° to the northwest of Messier 7, both north of the tail of Scorpius.

<span class="mw-page-title-main">Carina Nebula</span> Interstellar clouds in the constellation Carina

The Carina Nebula or Eta Carinae Nebula is a large, complex area of bright and dark nebulosity in the constellation Carina, located in the Carina–Sagittarius Arm of the Milky Way galaxy. The nebula is approximately 8,500 light-years (2,600 pc) from Earth.

<span class="mw-page-title-main">Messier 69</span> Globular cluster in the constellation Sagittarius

Messier 69 or M69, also known NGC 6637, is a globular cluster in the southern constellation of Sagittarius. It can be found 2.5° to the northeast of the star Epsilon Sagittarii and is dimly visible in 50 mm aperture binoculars. The cluster was discovered by Charles Messier on August 31, 1780, the same night he discovered M70. At the time, he was searching for an object described by Nicolas-Louis de Lacaille in 1751–2 and thought he had rediscovered it, but it is unclear if Lacaille actually described M69.

<span class="mw-page-title-main">NGC 3982</span> Galaxy in the constellation Ursa Major

NGC 3982(also known as UGC 6918) is an intermediate spiral galaxy approximately 68 million light-years away in the constellation Ursa Major. It was discovered by William Herschel on April 14, 1789, and misclassified as a planetary nebula. NGC 3982 is a part of the M109 Group.

<span class="mw-page-title-main">Sculptor Galaxy</span> Intermediate spiral galaxy in the constellation Sculptor

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<span class="mw-page-title-main">IC 2602</span> Open cluster in the constellation Carina

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<span class="mw-page-title-main">NGC 6231</span> Open Cluster in the constellation of Scorpius

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<span class="mw-page-title-main">NGC 2867</span> Planetary nebula in the constellation Carina

NGC 2867 is an elliptical Type II planetary nebula in the southern constellation of Carina, just over a degree to the NNW of the star Iota Carinae. It was discovered by John Herschel on April 1, 1834. Herschel initially thought he might have found a new planet, but on the following night he checked again and discovered it had not moved. The nebula is located at a distance of 7,270 light-years from the Sun.

<span class="mw-page-title-main">NGC 265</span> Open star cluster in the constellation Tucana

NGC 265 is an open cluster of stars in the southern constellation of Tucana. It is located in the Small Magellanic Cloud, a nearby dwarf galaxy. The cluster was discovered by English astronomer John Herschel on April 11, 1834. J. L. E. Dreyer described it as, "faint, pretty small, round", and added it as the 265th entry in his New General Catalogue.

<span class="mw-page-title-main">NGC 3242</span> Planetary nebula in the constellation Hydra

NGC 3242 is a planetary nebula located in the constellation Hydra.

References

  1. 1 2 3 "NGC 3532". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2010-05-23.
  2. 1 2 Robichon, N.; et al. (2005). "Open clusters with Hipparcos. I. Mean astrometric parameters". Astronomy and Astrophysics. 345: 471–484. arXiv: astro-ph/9903131 . Bibcode:1999A&A...345..471R.
  3. 1 2 Deep Sky Observer's Companion – the online database, DOCdb Lacaille II.10
  4. 1 2 Nemiroff, R.; Bonnell, J., eds. (26 February 2010). "Chasing Carina". Astronomy Picture of the Day . NASA . Retrieved 17 April 2016.
  5. 1 2 Hook, Richard (26 November 2014). "A Colourful Gathering of Middle-aged Stars". European Southern Observatory. ESO . Retrieved 17 April 2016.
  6. 1 2 Kramer, Miriam (26 November 2014). "Wishing Well Star Cluster Sparkles in Colorful New Views". Space.com. Space.com. Retrieved 17 April 2016.
  7. 1 2 Frommert, Hartmut; Kronberg, Christine (23 June 2006). "NGC 3532". SEDS Messier Database. SEDS. Retrieved 17 April 2016.
  8. 1 2 Martin Mobberley (Oct 2009). The Caldwell Objects and How to Observe Them. Springer. p. 190. ISBN   978-1-4419-0326-6.
  9. Stephen James O'Meara, The Caldwell Objects, Cambridge University Press, ISBN   0-521-82796-5, p. 358–360.
  10. Mike Inglis (July 2013). Observer's Guide to Star Clusters. Springer. p. 55. Bibcode:2013ogsc.book.....I. ISBN   978-1-4614-7567-5.
  11. Michael E. Bakich (July 2010). 1,001 Celestial Wonders to See Before You Die. Springer. p. 80. Bibcode:2010ocws.book.....B. ISBN   978-1-4419-1777-5.
  12. Amateur Astronomer Association of New York, Nebula of the Month - Carina's Football
  13. IceInSpace - Australian Amateur Astronomy, Challenge Objects - June 2005, 2005
  14. Chadwick, S; Cooper, I (11 December 2012). Imaging the Southern Sky. New York: Springer. p. 94. ISBN   978-1461447498.
  15. Claria, J.J., Lapasset, E., (1988) "A UBV and DDO astrophysical study of the open cluster NGC3532", Monthly Notices of the Royal Astronomical Society, 235, 1129–1139
  16. Reimers, D., Koester, D., (1989) "Spectroscopic identification of white dwarfs in galactic clusters. V - NGC 3532", Astronomy & Astrophysics, 218, 118–122
  17. Dobbie, P., Day-Jones, A., Williams, K., Casewell, S., Burleigh, M., Lodieu, N., Parker, Q., Baxter, R. (2012) "Further investigation of white dwarfs in the open clusters NGC2287 and NGC3532", Monthly Notices of the Royal Astronomical Society, 423, 2815–2828
  18. Jones, K. G. (March 1969). "The search for the nebulae - VI". Journal of the British Astronomical Association. 79: 213–222. Bibcode:1969JBAA...79..213J.
  19. Herschel, J. (1847). Results of Astronomical Observations Made During the Years 1834, 5, 6, 7, 8, at the Cape of Good Hope. London, Smith, Elder &Co.
  20. ScienceDaily, "A colorful gathering of middle-aged stars", European Southern Observatory, 26 November 2014
  21. 1 2 First Image Taken by Hubble's Wide Field Planetary Camera, Hubblesite.org
  22. "Great Exploration Revisited: New Horizons at Pluto and Charon".