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55 Cancri f

An artist's impression of 55 Cancri f. The three bright dots near its star are the three innermost planets.
Discovery
Discovered by	announced by J. Wisdom published by D. Fischer
Discovery site	United States
Discovery date	11 April 2005 (announced) 6 November 2007 (published)
Detection method	Doppler spectroscopy
Orbital characteristics
Apastron	0.833 AU (124,600,000 km)
Periastron	0.730 AU (109,200,000 km)
Semi-major axis	0.781 ± 0.007 AU (116,800,000 ± 1,000,000 km)
Eccentricity	0.2 ± 0.2
Orbital period (sidereal)	260.00 ± 1.1 d 0.7118 y
Time of periastron	2,450,080.9108 ± 1.1
Argument of periastron	181.1 ± 60
Semi-amplitude	4.879 ± 0.6
Star	55 Cancri A
Physical characteristics
Temperature	200–300 K (−73–27 °C; −100–80 °F)

55 Cancri f (abbreviated 55 Cnc f), also designated Rho Cancri f and formally named Harriot /ˈhæriət/, is an extrasolar planet approximately 41 light-years away from Earth in the constellation of Cancer (the Crab). 55 Cancri f is the fourth known planet (in order of distance) from the star 55 Cancri and the first planet to have been given the designation of "f".

Name

In July 2014 the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars. The process involved public nomination and voting for the new names. In December 2015, the IAU announced the winning name was Harriot for this planet. The winning name was submitted by the Royal Netherlands Association for Meteorology and Astronomy of the Netherlands. It honors the astronomer Thomas Harriot.

Discovery

The initial presentation of this planet occurred at a meeting of the American Astronomical Society in April 2005, however it was another two and a half years before the planet was to be published in a peer-reviewed journal. It is the first known planet outside our solar system to spend its entire orbit within what astronomers call the "habitable zone". Furthermore, its discovery made 55 Cancri the first star other than the Sun known to have at least five planets.

Orbit and mass

55 Cancri f is located about 0.781 AU away from the star and takes 262 days to complete a full orbit. A limitation of the radial velocity method used to detect 55 Cancri f is that only a minimum mass can be obtained, in this case around 0.144 times that of Jupiter, or half the mass of Saturn. A Keplerian fit to the radial velocity data of 55 Cancri A indicates that the orbit is consistent with being circular, however changing the value in a range between 0 and 0.4 does not significantly alter the chi-squared statistic of the fit, thus a representative eccentricity of 0.2±0.2 was assumed. In a Newtonian model which takes interactions between the planets into account, the eccentricity comes out as 0.0002, almost perfectly circular.

Astrometric observations made with the Hubble Space Telescope suggest that the outer planet 55 Cancri d is inclined at 53° with respect to the plane of the sky. The inner planets b and e are inclined at 85°. The inclination of f is unknown.

Characteristics

Since the planet was detected indirectly through observations of its star, properties such as its radius, composition and temperature are unknown. With a mass half that of Saturn, 55 Cancri f is likely to be a gas giant with no solid surface. It orbits in the so-called "habitable zone," which means that liquid water could exist on the surface of a possible moon.

It is not known if the composition and appearance is more like that of Saturn or Neptune. Based on its temperature, it could be a Sudarsky Class II planet, covered in water clouds, or a Sudarsky Class III with no clouds and a dark azure color.

References

1. ^ Debra A. Fischer; Geoffrey W. Marcy; R. Paul Butler; Steven S. Vogt; Greg Laughlin; Gregory W. Henry; et al. (23 December 2007). "Five Planets Orbiting 55 Cancri". Astrophysical Journal. 675: 790–801. arXiv:0712.3917. Bibcode:2008ApJ...675..790F. doi:10.1086/525512.
2. Mathematics Pronunciation Guide
3. ^ Shige Abe (12 November 2007). "Researchers Identify First Five-Planet Extrasolar System". NASA Astrobiology. Archived from the original on 16 September 2008. Retrieved 17 September 2008.
4. NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars. IAU.org. 9 July 2014
5. NameExoWorlds The Process
6. Final Results of NameExoWorlds Public Vote Released, International Astronomical Union, 15 December 2015.
7. NameExoWorlds The Approved Names
8. J. Wisdom (11 April 2005). "A Neptune-sized Planet in the rho Cancri System". DDA 36th Meeting, 10–14 April 2005—Session 5 Posters. The American Astronomical Society. Archived from the original on 16 December 2006. Retrieved 17 September 2008.
9. ^ Ian Sample, science correspondent (7 November 2007). "Could this be Earth's near twin? Introducing planet 55 Cancri f". The Guardian. London. Archived from the original on 2 October 2008. Retrieved 17 October 2008. {{cite news}}: |author= has generic name (help)
10. ^ Jean Schneider (2011). "Notes for Planet 55 Cnc f". Extrasolar Planets Encyclopaedia. Retrieved 8 October 2011.
11. Han; et al. (2001). "Preliminary Astrometric Masses for Proposed Extrasolar Planetary Companions". The Astrophysical Journal Letters. 548 (1): L57 – L60. Bibcode:2001ApJ...548L..57H. doi:10.1086/318927.

External links

Template:Misplaced Pages books

• Ward Glen (8 November 2007). "Astronomers Find Fifth Planet Around 55 Cancri". The Starry Mirror. Archived from the original on 10 November 2007. Retrieved 17 September 2008.

v t e The 55 Cancri system
55 Cancri A 55 Cancri B
55 Cancri e 55 Cancri b 55 Cancri c 55 Cancri f 55 Cancri d
See also binary stars extrasolar planets

• Use dmy dates from July 2013
• 55 Cancri
• Cancer (constellation)
• Exoplanets discovered in 2005
• Exoplanets detected by radial velocity
• Giant planets in the habitable zone
• Exoplanets with proper names