Mensa (constellation)

Mensa is a

One of the faintest constellations in the night sky, Mensa contains no apparently bright stars—the brightest,

History

Originally named "Montagne de la Table" or "Mons Mensae",^[1] Mensa was created by Nicolas-Louis de Lacaille out of dim Southern Hemisphere stars in honor of Table Mountain, a South African mountain overlooking Cape Town, near the location of Lacaille's observatory. He recalled that the Magellanic Clouds were sometimes known as Cape clouds, and that Table Mountain was often covered in clouds when a southeasterly stormy wind blew. Hence he made a "table" in the sky under the clouds.^[2] Lacaille had observed and catalogued 10,000 southern stars during a two-year stay at the Cape of Good Hope. He devised 14 new constellations in uncharted regions of the Southern Celestial Hemisphere not visible from Europe. Mensa was the only constellation that did not honor an instrument symbolic of the Age of Enlightenment.^[3] Sir John Herschel proposed shrinking the name to one word in 1844, noting that Lacaille himself had abbreviated some of his constellations thus.^[4]

Although the stars of Mensa do not feature in any ancient mythology, the mountain it is named after has a rich mythology. Called "Tafelberg" in Dutch and German, it has two neighboring mountains called "Devil's Peak" and "Lion's Head". Table Mountain features in the mythology of the Cape of Good Hope, notorious for its storms. Explorer Bartolomeu Dias saw the mountain as a mythical anvil for storms.

Characteristics

Mensa is bordered by

Bright stars

Lacaille gave eleven stars in the constellation Bayer designations, using the Greek alphabet to label them Alpha through to Lambda Mensae (excluding Kappa). Gould later added Kappa, Mu, Nu, Xi and Pi Mensae. Stars as dim as these were not generally given designations; however, Gould felt their closeness to the South Celestial Pole warranted their naming.^[2] Alpha Mensae is the brightest star with a barely visible apparent magnitude of 5.09,^[8] making it the only constellation with no star above magnitude 5.0.^[9] Overall, there are 22 stars within the constellation's borders brighter than or equal to apparent magnitude 6.5.^[b][5]

• Alpha Mensae is a
  projected separation of roughly 30 AU.^[8][15][16]
• Gamma Mensae is the second-brightest star in the constellation, at magnitude 5.19.^[17] Located 104.9 ± 0.5 light-years from Earth,^[11] it is an ageing (10.6 billion year-old) star around 1.04 times as massive as the Sun. It has swollen to around 5 times the solar radius,^[18] becoming an orange giant of spectral type K2III.^[19]
• Beta Mensae is slightly fainter at magnitude 5.31.^[17] Located 660 ± 10 light-years from Earth,^[11] it is a yellow giant of spectral type G8III, around 3.6 times as massive and 513 times as luminous as the Sun. It is 270 million years old,^[20] and lies in front of the Large Magellanic Cloud.^[17]
• Zeta and Eta Mensae have infrared excesses suggesting they too have circumstellar disks of dust.^[21][22] Zeta Mensae is an ageing white giant of spectral type A5 III around 394 ± 4 light-years from Earth,^[23][11] and Eta Mensae is an orange giant of spectral type K4 III,^[22] lying 650 ± 10 light-years away from Earth.^[11]
• Pi Mensae is a solar-type (G1) star 59.62 ± 0.07 light-years distant.^[11] In 2001, a substellar companion was discovered in an eccentric orbit.^[24] Incorporating more accurate Hipparcos data yields a mass range for the companion to be anywhere from 10.27 to 29.9 times that of Jupiter. This confirms its substellar nature with the upper limit of mass putting it in the brown dwarf range.^[25] The discovery of a second substellar companion—a super-Earth—was announced on 16 September 2018. It takes 6.27 days to complete its orbit and is the first exoplanet detected by the Transiting Exoplanet Survey Satellite (TESS) submitted for publication.^[26]

Planet-hosting stars

• HD 38283 (Bubup)^[27] is a Sun-like star of spectral type F9.5V of magnitude 6.7,^[28] located 124.3 ± 0.1 light-years distant.^[11] In 2011, a gas giant with an Earth-like orbital period of 363 days and a minimum mass a third that of Jupiter was discovered by the radial velocity method.^[28]
• HD 39194 is an orange dwarf of spectral type K0V and magnitude 8.08, located 86.21 ± 0.09 light-years distant.^[11] Three planets in close orbit were discovered by the High Accuracy Radial Velocity Planet Searcher (HARPS) in 2011. The three take 5.6, 14 and 34 days to complete an orbit around their star, and have minimum masses 3.72, 5.94 and 5.14 times that of the Earth respectively.^[29]

Variable stars

• TZ Mensae is an eclipsing binary that varies between magnitude 6.2 and 6.9 every 8.57 days.^[9] It is composed of two white main sequence stars in close orbit. One of these is of spectral type A0V, has a radius twice as that of the Sun and is 2.5 times as massive. The other, an A8V spectral type, has a radius 1.4 times that of the Sun and is 1.5 times as massive.^[30][31]
• UX Mensae is another eclipsing binary system composed of two young stars around 1.2 times as massive as the Sun and 2.2 ± 0.5 billion years of age,^[32] orbiting each other every 4.19 days.^[33] The system is 338.2 ± 0.9 light-years distant.^[11]
• TY Mensae is another eclipsing binary system classified as a W Ursae Majoris variable; the two components are so close that they share a common envelope of stellar material. The larger star has been calculated to be 1.86 times as massive, have 1.85 times the diameter and is 13.6 times as luminous, while the smaller is 0.4 times as massive, 0.84 times the diameter, and 1.7 times as luminous as the Sun. Their surface temperatures have been calculated at 8164 and 7183 K respectively.^[34]
• YY Mensae is an orange giant of spectral type K1III around 2.2 times as massive as the Sun, with 12.7 times its diameter and 70 times its luminosity. A rapidly rotating star with a period of 9.5 days, it is a strong emitter of X-rays and belongs to a class of star known as FK Comae Berenices variables.^[35] These stars are thought to have formed with the merger of two stars in a contact binary system.^[36] With an apparent magnitude of 8.05, it is 707 ± 6 light-years distant.^[11]
• cataclysmic variable star system composed of a white dwarf and a red dwarf that orbit each other every 2 hours 57 minutes. The stars are close enough that the white dwarf strips material off the red dwarf, creating an accretion disc that periodically ignites with a resulting brightening of the system.^[37]

• TU Mensae is another cataclysmic variable composed of a red dwarf and white dwarf. The orbital period of 2 hours 49 minutes is one of the longest for cataclysmic variable systems exhibiting brighter outbursts, known as superhumps. The normal outbursts result in an increase in brightness lasting around a day every 37 days, while the superhumps last 5–20 days and take place every 194 days.^[38]
• AO Mensae is a faint star of magnitude 9.8. An orange dwarf that has 80% the size and mass of the Sun,^[39] it is also a BY Draconis variable.^[40] These are a class of stars with starspots prominent enough that the star changes brightness as it rotates.^[41] It is a member of the Beta Pictoris moving group, a loose association of young stars moving across the galaxy.^[39]

Other stars

• spectral class cooler than Y1 located 47 ± 3 light-years away. Unable to be separated by observations to date, they are presumed to be of similar mass—8 to 20 times that of Jupiter—and are less than one AU apart.^[42]

The

References

Citations

• 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, VA: The McDonald & Woodward Publishing Company.
  ISBN 978-0939923786
  .

External links

Wikimedia Commons has media related to Mensa.

• The Deep Photographic Guide to the Constellations: Mensa
• The clickable Mensa