Three temperate Neptunes orbiting nearby stars

Fulton, Benjamin J. and Howard, Andrew W. and Weiss, Lauren M. and Sinukoff, Evan and Petigura, Erik A. and Isaacson, Howard and Hirsch, Lea and Marcy, Geoffrey W. and Henry, Gregory W. and Grunblatt, Samuel K. and Huber, Daniel and von Braun, Kaspar and Boyajian, Tabetha S. and Kane, Stephen R. and Wittrock, Justin and Horch, Elliott P. and Ciardi, David R. and Howell, Steve B. and Wright, Jason T. and Ford, Eric B. (2016) Three temperate Neptunes orbiting nearby stars. The Astrophysical Journal, 830 (1). pp. 46-64. ISSN 0004-637X

[img]
Preview
Text (Published Version)
Ciardi_2016_PV.pdf

Download (3390Kb) | Preview

Abstract

We present the discovery of three modestly irradiated, roughly Neptune-mass planets orbiting three nearby Solartype stars. HD 42618 b has a minimum mass of 15.4±2.4 M⊕, a semimajor axis of 0.55 au, an equilibrium temperature of 337 K, and is the first planet discovered to orbit the solar analogue host star, HD 42618. We also discover new planets orbiting the known exoplanet host stars HD 164922 and HD 143761 (p CrB). The new planet orbiting HD 164922 has a minimum mass of 12.9±1.6 M⊕ and orbits interior to the previously known Jovian mass planet orbiting at 2.1 au. HD 164922 c has a semimajor axis of 0.34 au and an equilibrium temperature of 418 K. HD 143761 c orbits with a semimajor axis of 0.44 au, has a minimum mass of 25±2 M⊕, and is the warmest of the three new planets with an equilibrium temperature of 445 K. It orbits exterior to the previously known warm Jupiter in the system. A transit search using space-based CoRoT data and ground-based photometry from the Automated Photometric Telescopes (APTs) at Fairborn Observatory failed to detect any transits, but the precise, high-cadence APT photometry helped to disentangle planetary-reflex motion from stellar activity. These planets were discovered as part of an ongoing radial velocity survey of bright, nearby, chromospherically inactive stars using the Automated Planet Finder (APF) telescope at Lick Observatory. The high-cadence APF data combined with nearly two decades of radial velocity data from Keck Observatory and gives unprecedented sensitivity to both short-period low-mass, and long-period intermediate-mass planets.


Statistics for USQ ePrint 32089
Statistics for this ePrint Item
Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Additional Information: Access to published version in accordance with the copyright policy of the publisher.
Faculty / Department / School: No Faculty
Date Deposited: 31 May 2017 05:50
Last Modified: 27 Jun 2017 04:28
Uncontrolled Keywords: planetary systems; stars: individual (HD 42618, HD 164922, HD 143761)
Fields of Research : 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Socio-Economic Objective: E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Identification Number or DOI: 10.3847/0004-637X/830/1/46
URI: http://eprints.usq.edu.au/id/eprint/32089

Actions (login required)

View Item Archive Repository Staff Only