Five planets orbiting 55 Cancri1

Debra A. Fischer, Geoffrey W. Marcy, R. Paul Butler, Steven S. Vogt, Greg Laughlin, Gregory W. Henry, David Abouav, Kathryn M.G. Peek, Jason T. Wright, John A. Johnson, Chris McCarthy, Howard Isaacson

Research output: Contribution to journalArticle

149 Citations (Scopus)

Abstract

We report 18 years of Doppler shift measurements of a nearby star, 55 Cancri, that exhibits strong evidence for five orbiting planets. The four previously reported planets are strongly confirmed here. A fifth planet is presented, with an apparent orbital period of 260 days, placing it 0.78 AU from the star in the large empty zone between two other planets. The velocity wobble amplitude of 4.9 m s-1 implies a minimum planet mass M sin i = 45.7 M. The orbital eccentricity is consistent with a circular orbit, but modest eccentricity solutions give similar xv2 fits. All five planets reside in low-eccentricity orbits, four having eccentricities under 0.1. The outermost planet orbits 5.8 AU from the star and has a minimum mass M sin i = 3.8 MJup, making it more massive than the inner four planets combined. Its orbital distance is the largest for an exoplanet with a well-defined orbit. The innermost planet has a semimajor axis of only 0.038 AU and has a minimum mass, M sin i, of only 10.8 M , making it one of the lowest mass exoplanets known. The five known planets within 6 AU define a minimum-mass protoplanetary nebula to compare with the classical minimum-mass solar nebula. Numerical N-body simulations show this system of five planets to be dynamically stable and show that the planets with periods of 14.65 and 44.3 days are not in a mean motion resonance. Millimagnitude photometry during 11 years reveals no brightness variations at any of the radial velocity periods, providing support for their interpretation as planetary.

Original languageEnglish (US)
Pages (from-to)790-801
Number of pages12
JournalAstrophysical Journal
Volume675
Issue number1
DOIs
StatePublished - Mar 1 2008

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planets
planet
eccentricity
extrasolar planets
orbits
stars
orbitals
solar nebula
circular orbits
nebulae
radial velocity
photometry
brightness
shift

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Fischer, D. A., Marcy, G. W., Butler, R. P., Vogt, S. S., Laughlin, G., Henry, G. W., ... Isaacson, H. (2008). Five planets orbiting 55 Cancri1. Astrophysical Journal, 675(1), 790-801. https://doi.org/10.1086/525512
Fischer, Debra A. ; Marcy, Geoffrey W. ; Butler, R. Paul ; Vogt, Steven S. ; Laughlin, Greg ; Henry, Gregory W. ; Abouav, David ; Peek, Kathryn M.G. ; Wright, Jason T. ; Johnson, John A. ; McCarthy, Chris ; Isaacson, Howard. / Five planets orbiting 55 Cancri1. In: Astrophysical Journal. 2008 ; Vol. 675, No. 1. pp. 790-801.
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Fischer, DA, Marcy, GW, Butler, RP, Vogt, SS, Laughlin, G, Henry, GW, Abouav, D, Peek, KMG, Wright, JT, Johnson, JA, McCarthy, C & Isaacson, H 2008, 'Five planets orbiting 55 Cancri1', Astrophysical Journal, vol. 675, no. 1, pp. 790-801. https://doi.org/10.1086/525512

Five planets orbiting 55 Cancri1. / Fischer, Debra A.; Marcy, Geoffrey W.; Butler, R. Paul; Vogt, Steven S.; Laughlin, Greg; Henry, Gregory W.; Abouav, David; Peek, Kathryn M.G.; Wright, Jason T.; Johnson, John A.; McCarthy, Chris; Isaacson, Howard.

In: Astrophysical Journal, Vol. 675, No. 1, 01.03.2008, p. 790-801.

Research output: Contribution to journalArticle

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Fischer DA, Marcy GW, Butler RP, Vogt SS, Laughlin G, Henry GW et al. Five planets orbiting 55 Cancri1. Astrophysical Journal. 2008 Mar 1;675(1):790-801. https://doi.org/10.1086/525512