Rasio, F. A. and Nicholson, P. D. and Shapiro, S. L. and Teukolsky, S. A. (1992) An observational test for the existence of a planetary system orbiting PSR1257 + 12. Nature, 355 (6358). pp. 325-326. ISSN 0028-0836. doi:10.1038/355325a0. https://resolver.caltech.edu/CaltechAUTHORS:20180606-165654476
Full text is not posted in this repository. Consult Related URLs below.
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20180606-165654476
Abstract
FOLLOWING the first report of an object of planetary mass orbiting a pulsar, Wolszczan and Frail have now reported the even more surprising discovery of two planet-size companions in orbit around the nearby millisecond pulsar PSR1257+12. The orbital periods of the two planets are about 98 days and 67 days, very close to a 3:2 ratio. Here we point out that, because of this near commensurability, the mutual gravitational perturbations of the two planets should produce not only small secular changes, but also larger periodic changes in their orbital elements. In particular, we find that changes in the eccentricities and orbital periods should become measurable within a few years. Such a measurement would help determine the three masses in the system and the inclinations of the orbits. More importantly, a detection of these changes, if they accord with the theoretical predictions presented here, would provide irrefutable confirmation that the periodic residuals observed by Wolszczan and Frail are indeed caused by orbiting planets, rather than some other effect. For the single planet-size object previously reported1 around the pulsar PS R1829–10, there is no dynamical test analogous to the one proposed here to confirm the planetary interpretation.
Item Type: | Article | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
Related URLs: |
| |||||||||
ORCID: |
| |||||||||
Additional Information: | © 1992 Nature Publishing Group. We thank A. Wolszczan for discussions and for communicating results before publication. We also thank J Lissauer for drawing our attention to the Hill's sphere constraint. This work has been supported in part by NSF and NASA grants to Cornell University. | |||||||||
Funders: |
| |||||||||
Issue or Number: | 6358 | |||||||||
DOI: | 10.1038/355325a0 | |||||||||
Record Number: | CaltechAUTHORS:20180606-165654476 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20180606-165654476 | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 86876 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
Deposited By: | George Porter | |||||||||
Deposited On: | 07 Jun 2018 21:45 | |||||||||
Last Modified: | 15 Nov 2021 20:43 |
Repository Staff Only: item control page