Fornax

This article is about a constellation of stars. For the Roman goddess, see Fornax (mythology).
Fornax
Constellation

Abbreviation For
Genitive Fornacis
Pronunciation /ˈfɔːrnæks/, genitive /fɔːrˈneɪsᵻs/
Symbolism the brazier
Right ascension 3
Declination −30
Family La Caille
Quadrant SQ1
Area 398 sq. deg. (41st)
Main stars 2
Bayer/Flamsteed
stars		 27
Stars with planets 7
Stars brighter than 3.00m 0
Stars within 10.00 pc (32.62 ly) 2
Brightest star α For (3.80m)
Nearest star LP 944-20
(16.20 ly, 4.97 pc)
Messier objects None
Meteor showers None
Bordering
constellations		 Cetus
Sculptor
Phoenix
Eridanus
Visible at latitudes between +50° and −90°.
Best visible at 21:00 (9 p.m.) during the month of December.

Fornax (/ˈfɔːrnæks/) is a constellation in the southern sky. Its name is Latin for furnace. It was named by French astronomer Nicolas Louis de Lacaille in 1756. Fornax is one of the 88 modern constellations.

History

Fornax Chemica can be seen below Cetus in this card from Urania's Mirror (1825).

The French astronomer Nicolas Louis de Lacaille first described the constellation in French as le Fourneau Chymique (the Chemical Furnace) with an alembic and receiver in his early catalogue,[1] before abbreviating it to le Fourneau on his planisphere in 1752,[2][3] after he had observed and catalogued almost 10,000 southern stars during a two-year stay at the Cape of Good Hope. He devised fourteen new constellations in uncharted regions of the Southern Celestial Hemisphere not visible from Europe. All but one honoured instruments that symbolised the Age of Enlightenment.[lower-alpha 1] Lacaille Latinised the name to Fornax Chimiae on his 1763 chart.[1]

Characteristics

The constellation Eridanus borders Fornax to the east, north and south, while Cetus, Sculptor and Phoenix gird it to the north, west and south respectively. Covering 397.5 square degrees and 0.964% of the night sky, it ranks 41sr of the 88 constellations in size,[4] The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is 'For'.[5] The official constellation boundaries, as set by Eugène Delporte in 1930, are defined by a polygon of 8 segments (illustrated in infobox). In the equatorial coordinate system, the right ascension coordinates of these borders lie between 01h 45m 24.18s and 03h 50m 21.34s, while the declination coordinates are between -23.76° and -39.58°.[6] The whole constellation is visible to observers south of latitude 50°N.[lower-alpha 2]

Features

The constellation Fornax as it can be seen by the naked eye.

Stars

Lacaille gave Bayer designations to 27 stars now named Alpha to Omega Fornacis, labelling two stars 3.5 degrees apart as Gamma, three stars Eta, two stars Iota, two Lambda and three Chi. Phi Fornacis was added by Gould, and Theta and Omicron were dropped by Gould and Baily respectively. Upsilon, too, was later found to be two stars and designated as such.[1] Overall, there are 59 stars within the constellation's borders brighter than or equal to apparent magnitude 6.5.[lower-alpha 3][4] However, there are no stars brighter than the fourth magnitude.[8]

Originally designated 12 Eridani by John Flamsteed, Alpha Fornacis was named by Lacaille as the brightest star in the new constellation.[1] It is a binary star that can be resolved by small amateur telescopes. With an apparent magnitude of 3.91, the primary is a yellow-white subgiant 1.21 times as massive as the Sun that has begun to cool and expand after exhausting its core hydrogen, having swollen to 1.9 times the Sun's radius. Of magnitude 6.5, the secondary star is 0.78 times as massive as the Sun. It has been identified as a blue straggler, and has either accumulated material from, or merged with, a third star in the past. It is a strong source of X-rays.[9] The system is 46.4 ± 0.3 light-years distant from Earth.[10]

Beta Fornacis is a yellow-hued giant star of magnitude 4.5, 169 light-years from Earth.[11]

LP 944-20 is a brown dwarf of spectral type M9 around 21 light-years distant from Earth.

Six star systems have been found to have planets' Lambda2 Fornacis is a star about 1.2 times as massive as the Sun that has a planet about as massive as Neptune discovered by doppler spectroscopy in 2009. The planet has an orbit of around 17.24 days.[12]

Deep-sky objects

Four globular clusters in Fornax.[13]

NGC 1049 is a globular cluster 500,000 light-years from Earth. It is in the Fornax Dwarf Galaxy.[14] NGC 1360 is a planetary nebula in Fornax with a magnitude of approximately 9.0, 978 light-years from Earth. Its central star is of magnitude 11.4, an unusually bright specimen. It is five times the size of the famed Ring Nebula in Lyra at 6.5 arcminutes. Unlike the Ring Nebula, NGC 1360 is clearly elliptical.[15]

The Fornax Dwarf galaxy is a dwarf galaxy that is part of the Local Group of galaxies. It is not visible in amateur telescopes, despite its relatively small distance of 500,000 light-years.[11]


NGC 1097 is a barred spiral galaxy in Fornax, about 60 million light-years from Earth. At magnitude 9, it is visible in medium amateur telescopes.[16] It is notable as a Seyfert galaxy with strong spectral emissions indicating ionized gases and a central supermassive black hole.

NGC 1365 is another barred spiral galaxy located at a distance of 60 million light-years from Earth. Like NGC 1097, it is also a Seyfert galaxy. Its bar is a center of star formation and shows extensions of the spiral arms' dust lanes. The bright nucleus indicates the presence of an active galactic nucleus - a galaxy with a supermassive black hole at the center, accreting matter from the bar.[17] It is a 10th magnitude galaxy associated with the Fornax Cluster.[16]

Fornax A is a radio galaxy with extensive radio lobes that corresponds to the optical galaxy NGC 1316, a 9th-magnitude galaxy.[11] One of the closer active galaxies to Earth at a distance of 80 million light-years, Fornax A appears in the optical spectrum as a large elliptical galaxy with dust lanes near its core. These dust lanes have caused astronomers to discern that it recently merged with a small spiral galaxy. Because it has a high rate of type Ia supernovae, NGC 1316 has been used to determine the size of the universe. The jets producing the radio lobes are not particularly powerful, giving the lobes a more diffuse, knotted structure due to interactions with the intergalactic medium.[17] Associated with this peculiar galaxy is an entire cluster of galaxies.[11]

Fornax has been the target of investigations into the furthest reaches of the universe. The Hubble Ultra Deep Field is located within Fornax, and the Fornax Cluster, a small cluster of galaxies, lies primarily within Fornax. At a meeting of the Royal Astronomical Society in Britain, a team from University of Queensland described 40 unknown "dwarf" galaxies in this constellation; follow-up observations with the Hubble Space Telescope and the European Southern Observatory's Very Large Telescope revealed that ultra compact dwarfs are much smaller than previously known dwarf galaxies, about 120 light-years (37 pc) across.[18]

UDFj-39546284 is a candidate protogalaxy located in Fornax,[19][20][21][22] although recent analyses have suggested it is likely to be a lower redshift source.[23][24]

Equivalents

In Chinese astronomy, the stars that correspond to Fornax are located within the White Tiger of the West (西方白虎, Xī Fāng Bái Hǔ).[25]

See also

Notes

  1. ↑ The exception is Mensa, named for the Table Mountain. The other thirteen (alongside Fornax) are Antlia, Caelum, Circinus, Horologium, Microscopium, Norma, Octans, Pictor, Pyxis, Reticulum, Sculptor and Telescopium.[1]
  2. ↑ While parts of the constellation technically rise above the horizon to observers between 50°N and 66°N, stars within a few degrees of the horizon are to all intents and purposes unobservable.[4]
  3. ↑ Objects of magnitude 6.5 are among the faintest visible to the unaided eye in suburban-rural transition night skies.[7]

References

  1. 1 2 3 4 5 Wagman, Morton (2003). Lost Stars: Lost, Missing and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others. Blacksburg, Virginia: The McDonald & Woodward Publishing Company. pp. 6–7, 152. ISBN 978-0-939923-78-6.
  2. ↑ Ridpath, Ian. "Lacaille's Southern Planisphere of 1756". Star Tales. Self-published. Retrieved 7 November 2016.
  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 [588].
  4. 1 2 3 Ridpath, Ian. "Constellations: Andromeda–Indus". Star Tales. Self-published. Retrieved 7 November 2016.
  5. ↑ Russell, Henry Norris (1922). "The New International Symbols for the Constellations". Popular Astronomy. 30: 469. Bibcode:1922PA.....30..469R.
  6. ↑ "Fornax, Constellation Boundary". The Constellations. International Astronomical Union. Retrieved 7 November 2016.
  7. ↑ Bortle, John E. (February 2001). "The Bortle Dark-Sky Scale". Sky & Telescope. Sky Publishing Corporation. Retrieved 7 November 2016.
  8. ↑ Ridpath, Ian. "Fornax". Star Tales. Self-published. Retrieved 7 November 2016.
  9. ↑ Fuhrmann, K.; Chini, R. (2015). "Multiplicity among F-type Stars. II". The Astrophysical Journal. 809 (1): 19. Bibcode:2015ApJ...809..107F. doi:10.1088/0004-637X/809/1/107. 107.
  10. ↑ van Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv:0708.1752Freely accessible. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
  11. 1 2 3 4 Ridpath & Tirion 2001, pp. 148-149.
  12. ↑ O’Toole, Simon; Tinney, C. G.; Butler, R. Paul; Jones, Hugh R. A.; Bailey, Jeremy; Carter, Brad D.; Vogt, Steven S.; Laughlin, Gregory; Rivera, Eugenio J. (2009). "A Neptune-mass Planet Orbiting the Nearby G Dwarf HD16417". The Astrophysical Journal. 697 (2): 1263–1268. arXiv:0902.4024Freely accessible. Bibcode:2009ApJ...697.1263O. doi:10.1088/0004-637X/697/2/1263.
  13. ↑ "Four globular clusters in Fornax". www.spacetelescope.org. ESA/Hubble. Retrieved 21 November 2014.
  14. ↑ Levy 2005, p. 176.
  15. ↑ Levy 2005, pp. 134-135.
  16. 1 2 Ridpath & Tirion, pp. 148-149.
  17. 1 2 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.
  18. ↑ Hilker M. et. al., 2007
  19. ↑ Wall, Mike (December 12, 2012). "Ancient Galaxy May Be Most Distant Ever Seen". Space.com. Retrieved December 12, 2012. 13.75 Big Bang - 0.38 = 13.37
  20. ↑ NASA, "NASA's Hubble Finds Most Distant Galaxy Candidate Ever Seen in Universe", 26 January 2011
  21. ↑ "Hubble finds a new contender for galaxy distance record". Space Telescope (heic1103 - Science Release). 26 January 2011. Retrieved 2011-01-27.
  22. ↑ HubbleSite, "NASA's Hubble Finds Most Distant Galaxy Candidate Ever Seen in Universe", STScI-2011-05, 26 January 2011
  23. ↑ "A Tentative Detection of an Emission Line at 1.6 mum for the z ~ 12 Candidate UDFj-39546284". The Astrophysical Journal. 765: L2. 2013. arXiv:1301.0317Freely accessible. Bibcode:2013ApJ...765L...2B. doi:10.1088/2041-8205/765/1/l2.
  24. ↑ "Photometric Constraints on the Redshift of z ~ 10 Candidate UDFj-39546284 from Deeper WFC3/IR+ACS+IRAC Observations over the HUDF". The Astrophysical Journal. 765: L16. 2013. arXiv:1211.3105Freely accessible. Bibcode:2013ApJ...765L..16B. doi:10.1088/2041-8205/765/1/l16.
  25. ↑ (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 10 日
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Coordinates: 03h 00m 00s, −30° 00′ 00″

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