The first H-band spectrum of the giant planet β Pictoris b
- Univ. of California, Los Angeles, CA (United States). Dept. of Physics and Astronomy; Univ. of Toronto, ON (Canada). Dunlap Inst. for Astronomy and Astrophysics
- Univ. of Arizona, Tucson, AZ (United States). Lunar and Planetary Lab.
- Univ. of California, Los Angeles, CA (United States). Dept. of Physics and Astronomy
- Univ. of California, Berkeley, CA (United States). Astronomy Dept.
- Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Princeton Univ., NJ (United States). Dept. of Astrophysical Sciences
- Gemini Observatory, La Serena (Chile)
- Arizona State Univ., Tempe, AZ (United States); Univ. of Exeter (United Kingdom)
- Univ. of California, Santa Cruz, CA (United States). Univ. of California Observatories/Lick Observatory
- Univ. of Montreal, Quebec (Canada). Observatoire du Mont-M'egantic and D'epartement de physique
- National Research Council of Canada, Victoria, BC (Canada)
- Gemini Observatory, Hilo, HI (United States)
- Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
- Univ. of Toronto, ON (Canada)
- Carl Sagan Center, Mountain View, CA (United States). SETI Inst.
- NASA Ames Research Center (ARC), Moffett Field, Mountain View, CA (United States)
- National Research Council of Canada, Victoria, BC (Canada)
- Univ. of Arizona, Tucson, AZ (United States). Steward Observatory
- American Museum of Natural History, New York, NY (United States). Dept. of Astrophysics
- Arizona State Univ., Tempe, AZ (United States). School of Earth and Space Exploration
- Space Telescope Science Inst., Baltimore, MD (United States)
- National Research Council of Canada, Victoria, BC (United States)
- Cornell Univ., Ithaca, NY (United States). Sibley School of Mechanical and Aerospace Engineering
- American Museum of Natural History, New York, NY (United States). Dept. of Astrophysics; Space Telescope Science Inst., Baltimore, MD (United States)
- Univ. of Georgia, Athens, GA (United States). Dept. of Physics and Astronomy
- California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Jet Propulsion Lab.
- Univ. of California, Santa Cruz, CA (United States). Dept. of Astronomy
- Johns Hopkins Univ., Baltimore, MD (United States). Dept. of Physics and Astronomy
Using the recently installed Gemini Planet Imager (GPI), we have obtained the first H-band spectrum of the planetary companion to the nearby young star β Pictoris. GPI is designed to image and provide low-resolution spectra of Jupiter-sized, self-luminous planetary companions around young nearby stars. These observations were taken covering the H band (1.65 μm). The spectrum has a resolving power of ~45 and demonstrates the distinctive triangular shape of a cool substellar object with low surface gravity. Using atmospheric models, we find an effective temperature of 1600-1700 K and a surface gravity of log (g) = 3.5-4.5 (cgs units). These values agree well with "hot-start" predictions from planetary evolution models for a gas giant with mass between 10 and 12 MJup and age between 10 and 20 Myr.
- Research Organization:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC52-07NA27344
- OSTI ID:
- 1249120
- Report Number(s):
- LLNL-JRNL-663580
- Journal Information:
- The Astrophysical Journal. Letters (Online), Vol. 798, Issue 1; ISSN 2041-8213
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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