Harriot (exoplanet)

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Exoplanet
Harriot

Artist's impression

Artist's impression
Constellation cancer
Position
equinox : J2000.0
Right ascension 08h 52m 35.81093s
declination + 28 ° 19 ′ 50.9511 ″
Orbit data
Central star Copernicus A
Major semi-axis 0.7733 ± 0.001 AU
eccentricity 0.08   +0.102−0.057
Period of circulation 260.91 ± 0.36 d
Further data
Dimensions 0.1479   +0.0219−0.0093 M J
distance 12.5 pc
method Radial velocity method
history
Date of discovery 2007
Catalog names
55 Cancri f, HD 75732 f

Harriot ( 55 Cancri f ) is an exoplanet orbiting component A of the binary star system Copernicus . It is the fourth planet in the system and the last to be discovered. Due to its high mass , it is probably a gas planet .

discovery

The proof of Harriot is based like with all others of the 55 Cancri system on measurements of the radial velocity of the central star . After analyzing the radial velocity curves, Jack Wisdom suspected the existence of the planet as early as 2005 and announced this in April at the meeting of the American Astronomical Society . The publication in a scientific journal followed a year and a half later. The calculations with the assumption of this fifth planet with an orbit in the large gap between the three narrow planets Janssen, Galileo and Brahe and the rather wide planet Lipperhey enabled an overall stable planetary system with low eccentricities of all planets, as it is according to the generally accepted theories Planet formation is plausible.

Radial velocity changes at 55 Cancri caused by 55 Cancri f.

Track properties

The planet orbits its star at a distance of approximately 0.781 astronomical units with an eccentricity of 0.2. Its orbit is hardly further than that of Venus . It completes a cycle every 260 days .

Physical Properties

Fantasy representation of Copernicus A with its fourth planet.

Harriot has a minimum mass of approx. 45.78 earth masses or 0.144 Jupiter masses. So it is at least about half as heavy as Saturn . At present, one can only speculate about its radius, chemical composition and surface temperatures. Most likely it is a gas planet with no solid surface. Based on the orbit and the luminosity of Copernicus A, it could be in the habitable zone , so that liquid water and theoretically life on a potential moon appear possible.

Origin of name

Like all exoplanets, Harriot was originally designated with the star's official name and a lowercase letter, according to the order in which it was discovered. After a public IAU competition , it was given an official name on December 15, 2015, after the English astronomer Thomas Harriot .

swell

  • Debra A. Fischer, Geoffrey W. Marcy, R. Paul Butler, et al .: Five Planets Orbiting 55 Cancri. The Astrophysical Journal, 675 (2008), pp. 790-801. doi: 10.1086 / 525512 , arxiv : 0712.3917

Web links

Commons : 55 Cancri f  - Collection of images, videos and audio files

Individual evidence

  1. Simbad
  2. a b c d e f Exoplanet.eu
  3. International Astronomical Union: NameExoWorlds - The Approved Names. Retrieved January 3, 2016 .