ON THE TRANSIT POTENTIAL OF THE PLANET ORBITING IOTA DRACONIS
Abstract
Most of the known transiting exoplanets are in short-period orbits, largely due to the bias inherent in detecting planets through the transit technique. However, the eccentricity distribution of the known radial velocity planets results in many of those planets having a non-negligible transit probability. One such case is the massive planet orbiting the giant star iota Draconis, a situation where both the orientation of the planet's eccentric orbit and the size of the host star inflate the transit probability to a much higher value than for a typical hot Jupiter. Here we present a revised fit of the radial velocity data with new measurements and a photometric analysis of the stellar variability. We provide a revised transit probability, an improved transit ephemeris, and discuss the prospects for observing a transit of this planet from both ground and space.
- Authors:
-
- NASA Exoplanet Science Institute, California Institute of Technology, MS 100-22, 770 South Wilson Avenue, Pasadena, CA 91125 (United States)
- ZAH-Landessternwarte, Koenigstuhl 12, 69117 Heidelberg (Germany)
- Center of Excellence in Information Systems, Tennessee State University, 3500 John A. Merritt Blvd., Box 9501, Nashville, TN 37209 (United States)
- Publication Date:
- OSTI Identifier:
- 21460013
- Resource Type:
- Journal Article
- Journal Name:
- Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 720; Journal Issue: 2; Other Information: DOI: 10.1088/0004-637X/720/2/1644; Journal ID: ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; GIANT STARS; JUPITER PLANET; ORBITS; PROBABILITY; RADIAL VELOCITY; PLANETS; STARS; VELOCITY
Citation Formats
Kane, Stephen R, Reffert, Sabine, Schwab, Christian, Bergmann, Christoph, Henry, Gregory W, Fischer, Debra, and Clubb, Kelsey I., E-mail: skane@ipac.caltech.ed. ON THE TRANSIT POTENTIAL OF THE PLANET ORBITING IOTA DRACONIS. United States: N. p., 2010.
Web. doi:10.1088/0004-637X/720/2/1644.
Kane, Stephen R, Reffert, Sabine, Schwab, Christian, Bergmann, Christoph, Henry, Gregory W, Fischer, Debra, & Clubb, Kelsey I., E-mail: skane@ipac.caltech.ed. ON THE TRANSIT POTENTIAL OF THE PLANET ORBITING IOTA DRACONIS. United States. https://doi.org/10.1088/0004-637X/720/2/1644
Kane, Stephen R, Reffert, Sabine, Schwab, Christian, Bergmann, Christoph, Henry, Gregory W, Fischer, Debra, and Clubb, Kelsey I., E-mail: skane@ipac.caltech.ed. 2010.
"ON THE TRANSIT POTENTIAL OF THE PLANET ORBITING IOTA DRACONIS". United States. https://doi.org/10.1088/0004-637X/720/2/1644.
@article{osti_21460013,
title = {ON THE TRANSIT POTENTIAL OF THE PLANET ORBITING IOTA DRACONIS},
author = {Kane, Stephen R and Reffert, Sabine and Schwab, Christian and Bergmann, Christoph and Henry, Gregory W and Fischer, Debra and Clubb, Kelsey I., E-mail: skane@ipac.caltech.ed},
abstractNote = {Most of the known transiting exoplanets are in short-period orbits, largely due to the bias inherent in detecting planets through the transit technique. However, the eccentricity distribution of the known radial velocity planets results in many of those planets having a non-negligible transit probability. One such case is the massive planet orbiting the giant star iota Draconis, a situation where both the orientation of the planet's eccentric orbit and the size of the host star inflate the transit probability to a much higher value than for a typical hot Jupiter. Here we present a revised fit of the radial velocity data with new measurements and a photometric analysis of the stellar variability. We provide a revised transit probability, an improved transit ephemeris, and discuss the prospects for observing a transit of this planet from both ground and space.},
doi = {10.1088/0004-637X/720/2/1644},
url = {https://www.osti.gov/biblio/21460013},
journal = {Astrophysical Journal},
issn = {0004-637X},
number = 2,
volume = 720,
place = {United States},
year = {Fri Sep 10 00:00:00 EDT 2010},
month = {Fri Sep 10 00:00:00 EDT 2010}
}