Puppis

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Puppis
Constellation
Puppis IAU.svg
AbbreviationPup
Genitive Puppis
Pronunciation /ˈpʌpɪs/ , genitive the same
Symbolismthe Poop Deck
Right ascension 7.5h
Declination −30°
QuadrantSQ2
Area 673 sq. deg. (20th)
Main stars 9
Bayer/Flamsteed
stars
76
Stars with planets 6
Stars brighter than 3.00m1
Stars within 10.00 pc (32.62 ly)3
Brightest star ζ Pup (Naos) (2.25 m )
Messier objects 3
Meteor showers Pi Puppids
Zeta Puppids
Puppid-Velids
Bordering
constellations
Monoceros
Pyxis
Vela
Carina
Pictor
Columba
Canis Major
Hydra
Visible at latitudes between +40° and −90°.
Best visible at 21:00 (9 p.m.) during the month of February.

Puppis ("stern") is a constellation in the southern sky. It was originally part of the traditional constellation of Argo Navis (the ship of Jason and the Argonauts), which was divided into three parts, the other two being Carina (the keel and hull), and Vela (the sails). Puppis is the largest of the three constellations in square degrees. It is one of the 88 modern constellations recognized by the International Astronomical Union.

Contents

History

The constellation of Argo Navis is recorded in Greek texts, derived from ancient Egypt around 1000 BC. According to Plutarch, its equivalent in Egyptian astronomy was the "Boat of Osiris". [1]

As Argo Navis was roughly 28% larger than the next largest constellation, Hydra, [2] it was sub-divided into three sections in 1752 by the French astronomer Nicolas Louis de Lacaille, including Puppis, which he referred to as "Argûs in puppi". Despite the division, Lacaille kept a single set of Bayer designations for the whole constellation, Argo. Therefore, Carina has the α, β, and ε, Vela has γ and δ, Puppis has ζ, and so on. [3] In 1844, John Herschel proposed complete dividing Argo Navis in accordance with Lacaille's divisions. [4] However, the constellation continued to be used into the 20th century, and officially received a three-letter designation alongside its divisions in 1922. [5] Puppis, along with Carina and Vela, was included in the list of modern IAU constellations in 1930. [6]

Features

The constellation Puppis as it can be seen by the naked eye PuppisCC.jpg
The constellation Puppis as it can be seen by the naked eye

Named stars

DesignationNameOriginMeaning
ζ Puppis Naos Greek ship
π Puppis Ahadi Arabichaving much promise
ρ Puppis Tureis Arabic shield
ξ Puppis Asmidiske Greekgunwale
HD 48265 Nosaxa Mocoví springtime

Planetary systems

Several extrasolar planet systems have been found around stars in the constellation Puppis, including:

Deep-sky objects

The NGC 2467 star-forming region A cosmic concoction in NGC 2467.jpg
The NGC 2467 star-forming region

As the Milky Way runs through Puppis, there are many open clusters in the constellation. M46 and M47 are two open clusters in the same binocular field. M47 can be seen with the naked eye under dark skies, and its brightest stars are 6th magnitude. Messier 93 (M93) is another open cluster somewhat to the south. NGC 2451 is a very bright open cluster containing the star c Puppis, and the near NGC 2477 is a good target for small telescopes. The star Pi Puppis is the main component of a bright group of stars known as Collinder 135.

M46 is a circular open cluster with an overall magnitude of 6.1 at a distance of approximately 5400 light-years from Earth. The planetary nebula NGC 2438 is superimposed; it is approximately 2900 light-years from Earth. M46 is classified as a Shapley class f and a Trumpler class III 2 m cluster. This means that it is a rich cluster that appears distinct from the star field. However, it is not at its center. The cluster's stars, numbering between 50 and 100, have a moderate range in brightness. [7]

See also

Related Research Articles

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<span class="mw-page-title-main">Argo Navis</span> Obsolete Southern constellation

Argo Navis, or simply Argo, is one of Ptolemy's 48 constellations, now a grouping of three IAU constellations. It is formerly a single large constellation in the southern sky. The genitive is "Argus Navis", abbreviated "Arg". Flamsteed and other early modern astronomers called it Navis, genitive "Navis", abbreviated "Nav".

<span class="mw-page-title-main">Antlia</span> Constellation in the Southern Celestial Hemisphere

Antlia is a constellation in the Southern Celestial Hemisphere. Its name means "pump" in Latin and Greek; it represents an air pump. Originally Antlia Pneumatica, the constellation was established by Nicolas-Louis de Lacaille in the 18th century. Its non-specific (single-word) name, already in limited use, was preferred by John Herschel then welcomed by the astronomic community which officially accepted this. North of stars forming some of the sails of the ship Argo Navis, Antlia is completely visible from latitudes south of 49 degrees north.

<span class="mw-page-title-main">Ara (constellation)</span> Constellation in the southern celestial hemisphere

Ara is a southern constellation between Scorpius, Telescopium, Triangulum Australe, and Norma. It was one of the Greek bulk described by the 2nd-century astronomer Ptolemy, and it remains one of the 88 modern constellations designated by the International Astronomical Union.

<span class="mw-page-title-main">Carina (constellation)</span> Constellation in the southern celestial hemisphere

Carina is a constellation in the southern sky. Its name is Latin for the keel of a ship, and it was the southern foundation of the larger constellation of Argo Navis until it was divided into three pieces, the other two being Puppis, and Vela.

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

Fornax is a constellation in the southern celestial hemisphere, partly ringed by the celestial river Eridanus. 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.

<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">Pyxis</span> Constellation in the southern celestial hemisphere

Pyxis is a small and faint constellation in the southern sky. Abbreviated from Pyxis Nautica, its name is Latin for a mariner's compass. Pyxis was introduced by Nicolas-Louis de Lacaille in the 18th century, and is counted among the 88 modern constellations.

<span class="mw-page-title-main">Vela (constellation)</span> Constellation in the southern celestial hemisphere

Vela is a constellation in the southern sky, which contains the Vela Supercluster. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis, which was later divided into three parts, the others being Carina and Puppis. With an apparent magnitude of 1.8, its brightest star is the hot blue multiple star Gamma Velorum, one component of which is the closest and brightest Wolf-Rayet star in the sky. Delta and Kappa Velorum, together with Epsilon and Iota Carinae, form the asterism known as the False Cross. 1.95-magnitude Delta is actually a triple or quintuple star system.

<span class="mw-page-title-main">Norma (constellation)</span> Constellation in the southern celestial hemisphere

Norma is a small constellation in the Southern Celestial Hemisphere between Ara and Lupus, one of twelve drawn up in the 18th century by French astronomer Nicolas-Louis de Lacaille and one of several depicting scientific instruments. Its name is Latin for normal, referring to a right angle, and is variously considered to represent a rule, a carpenter's square, a set square or a level. It remains one of the 88 modern constellations.

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

Circinus is a small, faint constellation in the southern sky, first defined in 1756 by the French astronomer Nicolas-Louis de Lacaille. Its name is Latin for compass, referring to the drafting tool used for drawing circles. Its brightest star is Alpha Circini, with an apparent magnitude of 3.19. Slightly variable, it is the brightest rapidly oscillating Ap star in the night sky. AX Circini is a Cepheid variable visible with the unaided eye, and BX Circini is a faint star thought to have been formed from the merger of two white dwarfs. Two sun-like stars have planetary systems: HD 134060 has two small planets, and HD 129445 has a Jupiter-like planet. Supernova SN 185 appeared in Circinus in 185 AD and was recorded by Chinese observers. Two novae have been observed more recently, in the 20th century.

<span class="mw-page-title-main">Pavo (constellation)</span> Constellation in the southern celestial hemisphere

Pavo is a constellation in the southern sky whose name is Latin for 'peacock'. Pavo first appeared on a 35-cm (14 in) diameter celestial globe published in 1598 in Amsterdam by Petrus Plancius and Jodocus Hondius and was depicted in Johann Bayer's star atlas Uranometria of 1603, and was likely conceived by Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman. French explorer and astronomer Nicolas-Louis de Lacaille gave its stars Bayer designations in 1756. The constellations Pavo, Grus, Phoenix and Tucana are collectively known as the "Southern Birds".

<span class="mw-page-title-main">Messier 46</span> Open cluster in the constellation Puppis

Messier 46 or M46, also known as NGC 2437, is an open cluster of stars in the slightly southern constellation of Puppis. It was discovered by Charles Messier in 1771. Dreyer described it as "very bright, very rich, very large." It is about 5,000 light-years away. There are an estimated 500 stars in the cluster with a combined mass of 453 M, and it is thought to be a mid-range estimate of 251.2 million years old.

HD 69830 is a yellow dwarf star located 41.0 light-years away in the constellation of Puppis. In 2005, the Spitzer Space Telescope discovered a narrow ring of warm debris orbiting the star. The debris ring contains substantially more dust than the Solar System's asteroid belt. In 2006, three extrasolar planets with minimum masses comparable to Neptune were confirmed in orbit around the star, located interior to the debris ring.

<span class="mw-page-title-main">Omicron Velorum</span> Variable star in the constellation Vela

Omicron Velorum is a star in the constellation Vela. It is the brightest member of the loose naked eye open cluster IC 2391, also known as the ο Velorum Cluster.

NGC 2423-3 is a red giant star approximately 3,040 light-years away in the constellation of Puppis. The star is part of the NGC 2423 open cluster. The star has an apparent magnitude of 10 and an absolute magnitude of zero, with a mass of 2.4 times the Sun. In 2007, it was proposed that an exoplanet orbits the star, but this is now doubtful.

k Puppis Star in the constellation Puppis

k Puppis is a Bayer designation given to an optical double star in the constellation Puppis, the two components being k1 Puppis and k2 Puppis.

HD 60532 b is an extrasolar planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 3.15 times more than Jupiter, orbits at 0.77 AU, and takes 201.83 days to revolve in an eccentric orbit. This planet was discovered on September 22, 2008 in La Silla Observatory using the HARPS spectrograph. On this same day, the second planet in this system, HD 60532 c, was discovered in a 1:3 orbital resonance.

HD 60532 c is an extrasolar planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 7.46 times more than Jupiter, orbits at 1.58 AU, and takes 607 days to revolve in an eccentric orbit. This planet was discovered on September 22, 2008 in La Silla Observatory using the HARPS spectrograph. On this same day, the second planet in this system, HD 60532 b, was discovered in a 3:1 orbital resonance.

<span class="mw-page-title-main">Omicron Puppis</span> Variable Star in the constellation Puppis

Omicron Puppis (ο Puppis) is candidate binary star system in the southern constellation of Puppis. It is visible to the naked eye, having a combined apparent visual magnitude of +4.48. Based upon an annual parallax shift of 2.30 mas as seen from Earth, it is located roughly 1,400 light years from the Sun.

References

  1. Barentine, John (2015). A History of Obsolete, Extinct, or Forgotten Star Lore. Springer. pp. 72–73. ISBN   978-3-319-22795-5 via Google Books.
  2. Ridpath, Ian. "Argo Navis". Star Tales.
  3. Wagman, M. (2003). Lost Stars: Lost, Missing, and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others. McDonald & Woodward Publishing Company. ISBN   978-0-939923-78-6.
  4. Herschel, J. F. W. (8 Mar 1844). "Further Remarks on the Revision of the Southern Constellations". Monthly Notices of the Royal Astronomical Society . 6 (5): 61–62. Bibcode:1844MNRAS...6...60R. doi: 10.1093/mnras/6.5.60 .
  5. Russell, Henry Norris (1922). "The New International Symbols for the Constellations" (PDF). Popular Astronomy . 30. John August Media, LLC: 471. Bibcode:1922PA.....30..469R. Archived from the original on 27 Mar 2023 via ADS.
  6. Delporte, E. (1930). Delimitation Scientifique des constellations (tables et cartes). Cambridge University Press. Bibcode:1930dsct.book.....D.
  7. Levy 2005, pp. 85–86.

Sources