The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
A Giant Planet Imaged in the Disk of the Young Star β Pictoris
Open accessAbstract
Planet Is Born: The 10-million-year-old star β Pictoris, has long been suspected to host a planet. Through images obtained with the Very Large Telescope, an array of four telescopes located in Chile, Lagrange et al. (p. 57 , published online 10 June) now confirm the presence of a young, giant planet, β Pictoris b, orbiting within the dusty disk that surrounds the star. β Pictoris b orbits closer to its star than Uranus and Neptune do to the Sun in our solar system. This orbital separation is consistent with the in situ formation of the planet via a core accretion mechanism. Thus, giant planets can form within a stellar dust disk in only a few million years.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Optical Images of an Exosolar Planet 25 Light-Years from Earth
Kalas, P., Graham, J. R., Chiang, E., Fitzgerald, M. P., Clampin, M., Kite, E. S., Stapelfeldt, K., Marois, C., & Krist, J. (2008) · Science · doi:10.1126/science.1166609 · Cited by 840
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
Cited by
A Major Asymmetric Dust Trap in a Transition Disk
van der Marel, N., van Dishoeck, E. F., Bruderer, S., Birnstiel, T., Pinilla, P., Dullemond, C. P., van Kempen, T. A., Schmalzl, M., Brown, J. M., Herczeg, G. J., et al. (2013) · Science · doi:10.1126/science.1236770 · Cited by 608
Fast spin of the young extrasolar planet β Pictoris b
Snellen, I. A. G., Brandl, B. R., de Kok, R. J., Brogi, M., Birkby, J., & Schwarz, H. (2014) · Nature · doi:10.1038/nature13253 · Cited by 416
Stellar and substellar companions of nearby stars from Gaia DR2: Binarity from proper motion anomaly
Kervella, P., Arenou, F., Mignard, F., & Thévenin, F. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201834371 · Cited by 399
SPECTRAL AND PHOTOMETRIC DIAGNOSTICS OF GIANT PLANET FORMATION SCENARIOS
Spiegel, D. S., & Burrows, A. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/745/2/174 · Cited by 398
Biller, B. A., Liu, M. C., Wahhaj, Z., Nielsen, E. L., Close, L. M., Dupuy, T. J., Hayward, T. L., Burrows, A., Chun, M., Ftaclas, C., et al. (2010) · The Astrophysical Journal · doi:10.1088/2041-8205/720/1/l82 · Cited by 147
Metadata
- Authors
- Lagrange, A.-M., Bonnefoy, M., Chauvin, G., Apai, D., Ehrenreich, D., Boccaletti, A., Gratadour, D., Rouan, D., Mouillet, D., Lacour, S., & Kasper, M.
- Venue
- Science
- Published
- 2010-07-02
- Volume
- 329
- Issue
- 5987
- Pages
- 57-59
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2087569457
- Cited by
- 902
- References
- 2
- FWCI
- 42.31
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: A Giant Planet Imaged in the Disk of the Young Star β Pictoris. https://app.cochat.ai/papers/10.1126/science.1187187
- The paper
- Lagrange, A.-M., Bonnefoy, M., Chauvin, G., Apai, D., Ehrenreich, D., Boccaletti, A., Gratadour, D., Rouan, D., Mouillet, D., Lacour, S., & Kasper, M. (2010). A Giant Planet Imaged in the Disk of the Young Star β Pictoris. Science. https://doi.org/10.1126/science.1187187
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
