Abstract / Description of output
We update the TrES-4 system parameters using high-precision HARPS-N radial-velocity measurements and new photometric light curves. A combined spectroscopic and photometric analysis allows us to determine a spectroscopic orbit with a semi-amplitude K = 51 ± 3 ± s-1. The derived mass of TrES-4b is found to be Mp = 0.49 ± 0.04 MJup, significantly lower than previously reported. Combined with the large radius (Rp = 1.84+0.08 -0.09 RJup) inferred from our analysis, TrES-4b becomes the transiting hot Jupiter with the second-lowest density known. We discuss several scenarios to explain the puzzling discrepancy in the mass of TrES-4b in the context of the exotic class of highly inflated transiting giant planets.
Original language | English |
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Article number | L15 |
Journal | Astronomy & Astrophysics |
Volume | 575 |
DOIs | |
Publication status | Published - 2015 |
Keywords / Materials (for Non-textual outputs)
- Planetary systems
- Stars: individual: TrES-4b
- Techniques: photometric
- Techniques: radial velocities
- Techniques: spectroscopic