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Cited by 773

The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.

The Use of Transit Timing to Detect Terrestrial-Mass Extrasolar Planets

Holman, Matthew J., Murray, Norman W.·2005·Science

Abstract

Future surveys for transiting extrasolar planets are expected to detect hundreds of jovian-mass planets and tens of terrestrial-mass planets. For many of these newly discovered planets, the intervals between successive transits will be measured with an accuracy of 0.1 to 100 minutes. We show that these timing measurements will allow for the detection of additional planets in the system (not necessarily transiting) by their gravitational interaction with the transiting planet. The transit-time variations depend on the mass of the additional planet, and in some cases terrestrial-mass planets will produce a measurable effect. In systems where two planets are seen to transit, the density of both planets can be determined without radial-velocity observations.

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Metadata

Authors
Holman, M. J., & Murray, N. W.
Venue
Science
Published
2005-02-25
Volume
307
Issue
5713
Pages
1288-1291
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2029806711
Cited by
773
References
23
FWCI
19.52
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The Use of Transit Timing to Detect Terrestrial-Mass Extrasolar Planets. https://app.cochat.ai/papers/10.1126/science.1107822
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Holman, M. J., & Murray, N. W. (2005). The Use of Transit Timing to Detect Terrestrial-Mass Extrasolar Planets. Science. https://doi.org/10.1126/science.1107822

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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.