请输入您要查询的百科知识:

 

词条 Caelum
释义

  1. History

  2. Characteristics

  3. Notable features

      Stars    Deep-sky objects  

  4. Notes

  5. References

  6. External links

{{short description|Constellation in the southern celestial hemisphere}}{{for|the cargo ship|USS Caelum (AK-106)}}{{Infobox constellation
| name = Caelum
| abbreviation = Cae
| genitive = Caeli[1]
| pronounce = {{IPAc-en|ˈ|s|iː|l|əm}}, genitive {{IPAc-en|ˈ|s|iː|l|aɪ}}
| symbolism = the chisel
| RA = {{RA|04|19.5}} to {{RA|05|05.1}}[2]
| dec= {{dec|−27.02}} to {{dec|−48.74}}[2]
| family = La Caille
| quadrant = SQ1
| areatotal = 125
| arearank = 81st
| numbermainstars = 4
| numberbfstars = 8
| numberstarsplanets = 1
| numberbrightstars = 0
| numbernearbystars = 0
| brighteststarname = α Cae
| starmagnitude = 4.45
| neareststarname = HD 30876
| stardistancely = 57.86
| stardistancepc = 17.75
| numbermessierobjects = 0
| meteorshowers = 1
| bordering = Columba
Lepus
Eridanus
Horologium
Dorado
Pictor
| latmax = 40
| latmin = 90
| month = January
| notes=}}

Caelum {{IPAc-en|ˈ|s|iː|l|əm}} is a faint constellation in the southern sky, introduced in the 1750s by Nicolas Louis de Lacaille and counted among the 88 modern constellations. Its name means “chisel” in Latin, and it was formerly known as Caelum Scalptorium (“the engravers’ chisel”); It is a rare word, unrelated to the far more common Latin caelum, meaning “sky, heaven, atmosphere”.[1] It is the eighth-smallest constellation, and subtends a solid angle of around 0.038 steradians, just less than that of Corona Australis.

Due to its small size and location away from the plane of the Milky Way, Caelum is a rather barren constellation, with few objects of interest. The constellation's brightest star, Alpha Caeli, is only of magnitude 4.45, and only one other star, (Gamma) γ 1 Caeli, is brighter than magnitude 5 . Other notable objects in Caelum are RR Caeli, a binary star with one known planet approximately {{convert|20.13|pc|ly}} away; X Caeli, a Delta Scuti variable that forms an optical double with γ 1 Caeli; and HE0450-2958, a Seyfert galaxy that at first appeared as just a jet, with no host galaxy visible.

History

Caelum was first introduced in the eighteenth century by Nicolas Louis de Lacaille, a French astronomer who introduced thirteen other southern constellations at the same time.[2]

Lacaille gave the constellation the French name Burin, which was originally Latinized to Caelum Scalptorium (“The Engravers’ Chisel”).

Francis Baily shortened this name to Caelum, as suggested by John Herschel.[3] In Lacaille's original chart, the constellation was shown both as a burin and an échoppe, although it has come to be recognized simply as a chisel.[3] Johann Elert Bode stated the name as plural with a singular possessor, Caela Scalptoris – in German (die ) Grabstichel (“the Engraver’s Chisels”) – but this did not stick.[8][4]

 

Characteristics

Caelum is bordered by Dorado and Pictor to the south, Horologium and Eridanus to the east, Lepus to the north, and Columba to the west. Covering only 125 square degrees, it ranks 81st of the 88 modern constellations in size. It appears prominently in the southern sky during the Southern Hemisphere's summer, and the whole constellation is visible for at least part of the year to observers south of latitude 41°N.[5]{{efn|1=While parts of the constellation technically rise above the horizon to observers between 41°N and 62°N, stars within a few degrees of the horizon are to all intents and purposes unobservable.[5]}}

Its main asterism consists of four stars, and twenty stars in total are brighter than magnitude 6.5 .[5]

The constellation's boundaries, as set by Eugène Delporte in 1930, are defined by a 12-sided polygon. In the equatorial coordinate system, the right ascension coordinates of these borders lie between {{RA|04|19.5}} and {{RA|05|05.1}}, while the declination coordinates are between {{dec|−27.02}} and {{dec|−48.74}}.[6] The International Astronomical Union (IAU) adopted the three-letter abbreviation “Cae” for the constellation in 1922.[7]

Notable features

Stars

{{See also|List of stars in Caelum}}

Caelum is a faint constellation: It has no star brighter than magnitude 4 and only two stars brighter than magnitude 5.

Lacaille gave six stars Bayer designations, labeling them Alpha (α ) to Zeta (ζ ) in 1756, but omitted Epsilon (ε ) and designated two adjacent stars as Gamma (γ ). Bode extended the designations to Rho (ρ ) for other stars, but most of these have fallen out of use.[8] Caelum is too far south for any of its stars to bear Flamsteed designations.{{efn|1=Southern constellations such as Caelum have no Flamsteed designations because Flamsteed only catalogued stars that were visible from England,.[9]|date=14 February 2014}}

The brightest star, (Alpha) α Caeli, is a double star, containing an F-type main-sequence star of magnitude 4.45 and a red dwarf of magnitude 12.5 , {{convert|20.17|pc|ly}} from Earth.[10][11] (Beta) β Caeli, another F-type star of magnitude 5.05 , is further away, being located {{convert|28.67|pc|ly}} from Earth. Unlike α, β Caeli is a subgiant star, slightly evolved from the main sequence.[12] (Delta) δ Caeli, also of magnitude 5.05 , is a B-type subgiant and is much farther from Earth, at {{convert|216|pc|ly}}.[13]

(Gamma) γ 1 Caeli is a double-star with a red giant primary of magnitude 4.58 and a secondary of magnitude 8.1 . The primary is {{convert|55.59|pc|ly}} from Earth. The two components are difficult to resolve with small amateur telescopes because of their difference in visual magnitude and their close separation.[14] This star system forms an optical double with the unrelated X Caeli (previously named γ 2 Caeli), a Delta Scuti variable located {{convert|98.33|pc|ly}} from Earth.[15] These are a class of short-period (six hours at most) pulsating stars that have been used as standard candles and as subjects to study astroseismology.[16] X Caeli itself is also a binary star, specifically a contact binary,[17] meaning that the stars are so close that they share envelopes. The only other variable star in Caelum visible to the naked eye is RV Caeli, a pulsating red giant of spectral type M1III,[18] which varies between magnitudes 6.44 and 6.56 .[19]

Three other stars in Caelum are still occasionally referred to by their Bayer designations, although they are only on the edge of naked-eye visibility. (Nu) ν Caeli[20] is another double star, containing a white giant of magnitude 6.07[21] and a star of magnitude 10.66, with unknown spectral type.[22] The system is approximately {{convert|52.55|pc|ly}} away.[21] (Lambda) λ Caeli,[23] at magnitude 6.24, is much redder and farther away, being a red giant around {{convert|227|pc|ly}} from Earth.[24] (Zeta) ζ Caeli is even fainter, being only of magnitude 6.36 . This star, located {{convert|132|pc|ly}} away, is a K-type subgiant of spectral type K1.[25] The other twelve naked-eye stars in Caelum are not referred to by Bode's Bayer designations anymore, including RV Caeli.

One of the nearest stars in Caelum is the eclipsing binary star RR Caeli, at a distance of {{convert|20.13|pc|ly}}.[34] This star system consists of a dim red dwarf and a white dwarf.[26] Despite its closeness to the Earth, the system's apparent magnitude is only 14.40[27] due to the faintness of its components, and thus it cannot be easily seen with amateur equipment. In 2012, the system was found to contain a giant planet, and there is evidence for a second substellar body.[28] The system is a post-common-envelope binary and is losing angular momentum over time, which will eventually cause mass transfer from the red dwarf to the white dwarf. In approximately 9–20 billion years, this will cause the system to become a cataclysmic variable.[29]

Deep-sky objects

Due to its small size and location away from the plane of the Milky Way, Caelum is rather devoid of deep-sky objects, and contains no Messier objects. The only deep-sky object in Caelum to receive much attention is HE0450-2958, an unusual Seyfert galaxy. Originally, the jet's host galaxy proved elusive to find, and this jet appeared to be emanating from nothing.[30] Although it has been suggested that the object is an ejected supermassive black hole,[31] the host is now agreed to be a small galaxy that is difficult to see due to light from the jet and a nearby starburst galaxy.[32]

Notes

{{notelist}}

References

1. ^Charlton T. Lewis, Ph.D. and. Charles Short, A Latin Dictionary Oxford University Press, 1879. Entries for caelum and caelum.
2. ^{{cite web|url = http://www.ianridpath.com/startales/lacaille.htm |work = Star Tales |title = Lacaille |last = Ridpath |first = Ian |accessdate=3 May 2014 |publisher=self-published}}
3. ^{{cite web |url = http://www.ianridpath.com/startales/caelum.htm |work = Star Tales |title = Caelum |last = Ridpath |first = Ian |accessdate=3 May 2014 |publisher=self-published}}
4. ^J. E. Bode: Allgemeine Beschreibung und Nachweisung der Gestirne nebst Verzeichniß der geraden Aufsteigung und Abweichung von 17240 Sternen, Doppelsternen, Nebelflecken und Sternhaufen. Berlin, 1801, p.17
5. ^{{cite web| url=http://www.ianridpath.com/constellations1.htm | title=Constellations: Andromeda–Indus | work= Star Tales |last=Ridpath |first=Ian |authorlink=Ian Ridpath |publisher=self-published | accessdate= 1 April 2014}}
6. ^{{cite journal | title=Caelum, Constellation Boundary | journal=The Constellations | publisher=International Astronomical Union | url=http://www.iau.org/public/constellations/#cae|accessdate=14 January 2014}}
7. ^{{cite journal | last=Russell | first=H. N.| title=The New International Symbols for the Constellations | journal=Popular Astronomy | volume=30 |pages=469–71 |bibcode=1922PA.....30..469R | year=1922}}
8. ^{{cite book | last = Wagman | first = Morton | year = 2003 | title = Lost Stars: Lost, Missing, and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others | publisher = The McDonald & Woodward Publishing Company | location = Blacksburg, VA | isbn = 978-0-939923-78-6 |pages=58–59}}
9. ^{{cite web |last1=Kaler |first1=J. B. |title=Star Names |publisher=University of Illinois at Urbana–Champaign |accessdate=11 May 2014 |url=http://stars.astro.illinois.edu/sow/starname.html}}
10. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=alf+Cae |title = * Alpha Caeli – Star in double system|publisher = SIMBAD | accessdate = 13 January 2013}}
11. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=CCDM%20J04406-4152%20B |title = GJ 174.1 B – Flare star|publisher = SIMBAD | accessdate = 13 January 2013}}
12. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=bet+Cae |title = LTT 2063 – High proper-motion Star|publisher = SIMBAD | accessdate = 13 January 2013}}
13. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=del+Cae |title = * Delta Caeli – Star|publisher = SIMBAD | accessdate = 13 January 2013}}
14. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=gam+Cae |title = * Gamma Caeli – Star|publisher = SIMBAD | accessdate = 13 January 2013}}
15. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=X+Cae |title = V* X Caeli – Variable Star of Delta Scuti type|publisher = SIMBAD | accessdate = 13 January 2013}}
16. ^{{cite web|url=http://www.aavso.org/vsots_delsct|title=Delta Scuti and the Delta Scuti Variables|last=Templeton|first=M. |date=16 July 2010|work=AAVSO Website|publisher=American Association of Variable Star Observers|accessdate=2 February 2014}}
17. ^{{cite web|url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=4518 |title=X Caeli |last1=X. |first1=V. S. |last2=Patrick |first2=W. |date=4 January 2010 |work=AAVSO Website|publisher=American Association of Variable Star Observers|accessdate=28 March 2014}}
18. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=RV+Cae |title = V* RV Caeli – Pulsating variable Star |publisher = SIMBAD | accessdate = 17 January 2013}}
19. ^{{cite web|url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=4525 |title=RV Caeli |last1=X. |first1=V. S. |date=25 August 2009|work=AAVSO Website|publisher=American Association of Variable Star Observers|accessdate=3 February 2014}}
20. ^{{cite web|author=Ashland Astronomy Studio: Where Art and Science Converge|title=Nu Caeli (HIP 22488)|url=http://www.astrostudio.org/xhip.php?hip=22488|accessdate=15 January 2014|deadurl=yes|archiveurl=https://web.archive.org/web/20140129110728/http://www.astrostudio.org/xhip.php?hip=22488|archivedate=29 January 2014|df=}}
21. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD+30985 |title = HR 1557 – Star in double system |publisher = SIMBAD | accessdate = 15 January 2013}}
22. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=CD-41%20%201593B |title = CD-41 1593B – Star in double system |publisher = SIMBAD | accessdate = 15 January 2013}}
23. ^{{cite web|author=Ashland Astronomy Studio: Where Art and Science Converge|title=Lambda Caeli (HIP 21998)|url=http://www.astrostudio.org/xhip.php?hip=21998|accessdate=15 January 2014|deadurl=yes|archiveurl=https://web.archive.org/web/20140129110726/http://www.astrostudio.org/xhip.php?hip=21998|archivedate=29 January 2014|df=}}
24. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HR+1518 |title = HR 1518 – Star |publisher = SIMBAD | accessdate = 15 January 2013}}
25. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=zet+Cae |title = Zeta Caeli – Star |publisher = SIMBAD | accessdate = 15 January 2013}}
26. ^{{Cite journal | last1 = Bruch | first1 = A. | last2 = Diaz | first2 = M. P. | doi = 10.1086/300471 | title = The Eclipsing Precataclysmic Binary RR Caeli | journal = The Astronomical Journal | volume = 116 | issue = 2 | pages = 908 | year = 1998 | pmid = | pmc = |bibcode = 1998AJ....116..908B }}
27. ^{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?Ident=RR+Cae |title = V* RR Caeli – Eclipsing binary of Algol type (detached) |publisher = SIMBAD | accessdate = 15 January 2013}}
28. ^{{Cite journal | last1 = Qian | first1 = S. B. | last2 = Liu | first2 = L. | last3 = Zhu | first3 = L. Y. | last4 = Dai | first4 = Z. B. | last5 = Fernández Lajús | first5 = E. | last6 = Baume | first6 = G. L. | doi = 10.1111/j.1745-3933.2012.01228.x | title = A circumbinary planet in orbit around the short-period white dwarf eclipsing binary RR Cae | journal = Monthly Notices of the Royal Astronomical Society: Letters | volume = 422 | issue = 1 | pages = L24–L27 | year = 2012 | pmid = | pmc = |arxiv = 1201.4205 |bibcode = 2012MNRAS.422L..24Q }}
29. ^{{Cite journal | last1 = Maxted | first1 = P. F. L. | last2 = O'Donoghue | first2 = D. | last3 = Morales-Rueda | first3 = L. | last4 = Napiwotzki | first4 = R. | last5 = Smalley | first5 = B. | title = The mass and radius of the M-dwarf in the short-period eclipsing binary RR Caeli | doi = 10.1111/j.1365-2966.2007.11564.x| bibcode= 2007MNRAS.376..919M | arxiv = astro-ph/0702005| journal = Monthly Notices of the Royal Astronomical Society | volume = 376 | issue = 2 | pages = 919–928| year = 2007 | pmid = | pmc = }}
30. ^{{Cite journal | last1 = Magain | first1 = P. | last2 = Letawe | first2 = G. R. | last3 = Courbin | first3 = F. D. R. | last4 = Jablonka | first4 = P. | last5 = Jahnke | first5 = K. | last6 = Meylan | first6 = G. | last7 = Wisotzki | first7 = L. | doi = 10.1038/nature04013 | title = Discovery of a bright quasar without a massive host galaxy | journal = Nature | volume = 437 | issue = 7057 | pages = 381–384 | year = 2005 | pmid = 16163349| pmc = |arxiv = astro-ph/0509433 |bibcode = 2005Natur.437..381M }}
31. ^{{Cite journal | last1 = Haehnelt | first1 = M. G. | last2 = Davies | first2 = M. B. | last3 = Rees | first3 = M. J. | title = Possible evidence for the ejection of a supermassive black hole from an ongoing merger of galaxies | doi = 10.1111/j.1745-3933.2005.00124.x | journal = Monthly Notices of the Royal Astronomical Society: Letters | volume = 366 | issue = 1 | pages = L22–L25 | year = 2006 | pmid = | pmc = |arxiv = astro-ph/0511245 |bibcode = 2006MNRAS.366L..22H }}
32. ^{{Cite journal | last1 = Feain | first1 = I. J. | last2 = Papadopoulos | first2 = P. P. | last3 = Ekers | first3 = R. D. | last4 = Middelberg | first4 = E. | title = Dressing a Naked Quasar: Star Formation and Active Galactic Nucleus Feedback in HE 0450−2958 | doi = 10.1086/518027 | journal = The Astrophysical Journal | volume = 662 | issue = 2 | pages = 872 | year = 2007 | pmid = | pmc = |arxiv = astro-ph/0703101 |bibcode = 2007ApJ...662..872F }}

External links

{{commons|Caelum}}
  • Starry Night Photography – Caelum Constellation
{{Stars of Caelum}}{{navconstel}}{{ConstellationsByLacaille}}{{Sky|05|00|00|-|40|00|00|10}}{{Featured article}}

3 : Caelum|Southern constellations|Constellations listed by Lacaille

随便看

 

开放百科全书收录14589846条英语、德语、日语等多语种百科知识,基本涵盖了大多数领域的百科知识,是一部内容自由、开放的电子版国际百科全书。

 

Copyright © 2023 OENC.NET All Rights Reserved
京ICP备2021023879号 更新时间:2024/11/17 16:59:47