The DOI matches its Crossref record; 19 of the 20 references it cites were found in a registry or an index.
Optical Images of an Exosolar Planet 25 Light-Years from Earth
Open accessAbstract
Fomalhaut, a bright star 7.7 parsecs (25 light-years) from Earth, harbors a belt of cold dust with a structure consistent with gravitational sculpting by an orbiting planet. Here, we present optical observations of an exoplanet candidate, Fomalhaut b. Fomalhaut b lies about 119 astronomical units (AU) from the star and 18 AU of the dust belt, matching predictions of its location. Hubble Space Telescope observations separated by 1.73 years reveal counterclockwise orbital motion. Dynamical models of the interaction between the planet and the belt indicate that the planet's mass is at most three times that of Jupiter; a higher mass would lead to gravitational disruption of the belt, matching predictions of its location. The flux detected at 0.8 μm is also consistent with that of a planet with mass no greater than a few times that of Jupiter. The brightness at 0.6 μm and the lack of detection at longer wavelengths suggest that the detected flux may include starlight reflected off a circumplanetary disk, with dimension comparable to the orbits of the Galilean satellites. We also observe variability of unknown origin at 0.6 μm.
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In the citing paper
“While the detected object is in orbit about Fomalhaut, its color is consistent with that of reflected light from the star.”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Kalas et al. 2008
In the citing paper
“The planet Fomalhaut b has been detected in two visible bands only (Kalas et al. 2008).”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Kalas et al. 2008
In the citing paper
“These observations led Kalas et al. to suggest that the planet hosts a circumplanetary ring akin to Saturn's (see Arnold & Schneider 2004), which would extend to at least 20 Jupiter radii for an assumed albedo of 0.4 to recover the observed fluxes.”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Kalas et al. 2008
Citations
Cites
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Collisional model of asteroids and their debris
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A model of accretion disks in close binaries
Paczyński, B. (1977) · The Astrophysical Journal · doi:10.1086/155526 · Cited by 412
A planetary system as the origin of structure in Fomalhaut's dust belt
Kalas, P., Graham, J. R., & Clampin, M. (2005) · Nature · doi:10.1038/nature03601 · Cited by 411
Self-citationWyatt, M. C., Dermott, S. F., Telesco, C. M., Fisher, R. S., Grogan, K., Holmes, E. K., & Pina, R. K. (1999) · The Astrophysical Journal · doi:10.1086/308093 · Cited by 410
A planet on an inclined orbit as an explanation of the warp in the β Pictoris disc
Mouillet, D., Larwood, J. D., Papaloizou, J. C. B., & Lagrange, A. ‐. (1997) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/292.4.896 · Cited by 327
Beyond the T Dwarfs: Theoretical Spectra, Colors, and Detectability of the Coolest Brown Dwarfs
Burrows, A. S., Sudarsky, D., & Lunine, J. I. (2003) · The Astrophysical Journal · doi:10.1086/377709 · Cited by 301
Fortney, J. J., Marley, M. S., Saumon, D., & Lodders, K. (2008) · The Astrophysical Journal · doi:10.1086/589942 · Cited by 260
Flagged first, then by citations
1 of the 20 references couldn’t be matched to a known paper.
Research works printed but not linked: 3
- D. E. Backman, F. C. Gillett, in Cool Stars, Stellar Systems and the Sun, J. L. Linsky, R. E. Stencel, Eds. (Springer-Verlag, Berlin, 1987), pp. 340–350.
- D. Barrado y Navascues, Astron. Astrophys.339, 831 (1998).
- E. Chiang E. Kite P. Kalas J R. Graham M. Clampin Astrophys. J. in press; http://arxiv.org/abs/0811.1985. · arXiv
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Direct Imaging of Multiple Planets Orbiting the Star HR 8799
Marois, C., Macintosh, B., Barman, T., Zuckerman, B., Song, I., Patience, J. L., Lafreniére, D., & Doyon, R. (2008) · Science · doi:10.1126/science.1166585 · Cited by 1,711
Self-citationDuchêne, G., & Kraus, A. L. (2013) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102602 · Cited by 1,353
A Giant Planet Imaged in the Disk of the Young Star β Pictoris
Lagrange, A. ‐., Bonnefoy, M., Chauvin, G., Apai, D., Ehrenreich, D., Boccaletti, A., Gratadour, ., Rouan, D., Mouillet, D., Lacour, S., et al. (2010) · Science · doi:10.1126/science.1187187 · Cited by 901
Efficient, uninformative sampling of limb darkening coefficients for two-parameter laws
Kipping, D. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1435 · Cited by 927
Rapid growth of gas-giant cores by pebble accretion
Lambrechts, M., & Johansen, A. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201219127 · Cited by 923
Metadata
- Authors
- Kalas, P., Graham, J. R., Chiang, E., Fitzgerald, M. P., Clampin, M., Kite, E. S., Stapelfeldt, K., Marois, C., & Krist, J.
- Affiliations
- California Institute of Technology (US)
- Corresponding author
- Kalas, Paul
- ORCID
- Venue
- Science
- Published
- 2008-11-28
- Volume
- 322
- Issue
- 5906
- Pages
- 1345-1348
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2024605337
- Cited by
- 840
- References
- 20
- Citations by year
- 2026: 4 · 2025: 10 · 2024: 10 · 2023: 21 · 2022: 7 · 2021: 13 · 2020: 27 · 2019: 20 · 2018: 34 · 2017: 35 · 2016: 66 · 2015: 46 · 2014: 70 · 2013: 89 · 2012: 84
- FWCI
- 59.09
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Science (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- NASA STI Repository (National Aeronautics and Space Administration) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- Fomalhaut b, exoplanet detection, Fomalhaut, debris disks, gravitational perturbations, orbital motion, planet mass limits, circumplanetary disks, reflected starlight, optical photometry, Hubble Space Telescope, dynamic modeling
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