Obliquity of an Earth-like Planet from Frequency Modulation of Its Direct-imaged Lightcurve: Mock Analysis from General Circulation Model Simulation
| dc.contributor.author | NAKAGAWA, Yuta | |
| hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
| dc.contributor.author | KODAMA, Takanori | |
| dc.contributor.author | ISHIWATARI, Masaki | |
| dc.contributor.author | KAWAHARA, Hajime | |
| dc.contributor.author | SUTO, Yasushi | |
| dc.contributor.author | TAKAHASHI, Yoshiyuki O. | |
| dc.contributor.author | HASHIMOTO, George L. | |
| dc.contributor.author | KURAMOTO, Kiyoshi | |
| dc.contributor.author | NAKAJIMA, Kensuke | |
| dc.contributor.author | TAKEHIRO, Shin-Ichi | |
| dc.contributor.author | HAYASHI, Yoshi-Yuki | |
| dc.date.issued | 2020 | |
| dc.identifier.issn | 0004-637X | |
| dc.description.abstractEn | Direct-imaging techniques of exoplanets have made significant progress recently and will eventually enable monitoring of photometric and spectroscopic signals of Earth-like habitable planets. The presence of clouds, however, would remain as one of the most uncertain components in deciphering such direct-imaged signals of planets. We attempt to examine how the planetary obliquity produces different cloud patterns by performing a series of general circulation model simulation runs using a set of parameters relevant for our Earth. Then we use the simulated photometric lightcurves to compute their frequency modulation that is due to the planetary spin-orbit coupling over an entire orbital period, and we attempt to see to what extent one can estimate the obliquity of an Earth twin. We find that it is possible to estimate the obliquity of an Earth twin within the uncertainty of several degrees with a dedicated 4 m space telescope at 10 pc away from the system if the stellar flux is completely blocked. While our conclusion is based on several idealized assumptions, a frequency modulation of a directly imaged Earth-like planet offers a unique methodology to determine its obliquity. | |
| dc.language.iso | en | |
| dc.publisher | American Astronomical Society | |
| dc.subject.en | Exoplanet atmospheres | |
| dc.subject.en | Exoplanet surface composition | |
| dc.subject.en | Hydrodynamics | |
| dc.subject.en | Radiative transfer | |
| dc.subject.en | Oblique rotators | |
| dc.subject.en | Biosignatures | |
| dc.subject.en | Direct imaging | |
| dc.subject.en | Stellar photometry | |
| dc.subject.en | Earth atmosphere | |
| dc.subject.en | Atmospheric circulation | |
| dc.subject.en | 487 | |
| dc.subject.en | 2022 | |
| dc.subject.en | 1963 | |
| dc.subject.en | 1335 | |
| dc.subject.en | 1144 | |
| dc.subject.en | 2018 | |
| dc.subject.en | 387 | |
| dc.subject.en | 1620 | |
| dc.subject.en | 437 | |
| dc.subject.en | 112 | |
| dc.subject.en | Astrophysics - Earth and Planetary Astrophysics | |
| dc.subject.en | Astrophysics - Instrumentation and Methods for Astrophysics | |
| dc.subject.en | Astrophysics - Solar and Stellar Astrophysics | |
| dc.title.en | Obliquity of an Earth-like Planet from Frequency Modulation of Its Direct-imaged Lightcurve: Mock Analysis from General Circulation Model Simulation | |
| dc.type | Article de revue | |
| dc.identifier.doi | 10.3847/1538-4357/ab9eb8 | |
| dc.subject.hal | Planète et Univers [physics] | |
| dc.identifier.arxiv | 2006.11437 | |
| bordeaux.journal | The Astrophysical Journal | |
| bordeaux.volume | 898 | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | insu-03678865 | |
| hal.version | 1 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//insu-03678865v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=The%20Astrophysical%20Journal&rft.date=2020&rft.volume=898&rft.eissn=0004-637X&rft.issn=0004-637X&rft.au=NAKAGAWA,%20Yuta&KODAMA,%20Takanori&ISHIWATARI,%20Masaki&KAWAHARA,%20Hajime&SUTO,%20Yasushi&rft.genre=article |
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