Detecting companions to extrasolar planets using mutual events
arXiv:astro-ph/0703609 · doi:10.1051/0004-6361:20066111
Abstract
We investigate a new approach to the detection of companions to extrasolar planets beyond the transit method. We discuss the possibility of the existence of binary planets. We develop a method based on the imaging of a planet-companion as an unresolved system (but resolved from its parent star). It makes use of planet-companion mutual phenomena, namely mutual transits and mutual shadows. We show that companions can be detected and their radius measured down to lunar sizes.
6 pages, 7 figures
References in corpus (9)
- HST Time-Series Photometry of the Transiting Planet of HD 209458
- The Interiors of Giant Planets: Models and Outstanding Questions
- Stability of Satellites Around Close-in Extrasolar Giant Planets
- Characterization of extrasolar terrestrial planets from diurnal photometric variability
- Simulation of a Space-Based Microlensing Survey for Terrestrial Extra-Solar Planets
- Transit Detectability of Ring Systems Around Extrasolar Giant Planets
- On the Feasibility of Detecting Satellites of Extrasolar Planets via Microlensing
- The detectability of extrasolar planet surroundings - I. Reflected-light photometry of unresolved rings
- Terrestrial Exoplanet Light Curves
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- Defining and cataloging exoplanets: The exoplanet.eu database
- STARRY: Analytic Occultation Light Curves
- Transit timing effects due to an exomoon
- How to Characterize Habitable Worlds and Signs of Life
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- A Study of the Accuracy of Mass-Radius Relationships for Silicate-Rich and Ice-Rich Planets up to 100 Earth Masses
- Evidence for a Large Exomoon Orbiting Kepler-1625b
- Exomoon habitability constrained by illumination and tidal heating
- Formation, Habitability, and Detection of Extrasolar Moons
- On the detectability of habitable exomoons with Kepler-class photometry
- HEK VI: On the Dearth of Galilean Analogs in Kepler and the Exomoon Candidate Kepler-1625b I
- Characterizing Habitable Exo-Moons
- Outcomes and Duration of Tidal Evolution in a Star-Planet-Moon System
- The far future of exoplanet direct characterization
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- The Center of Light: Spectroastrometric Detection of Exomoons
- Modeling the Infrared Spectrum of the Earth-Moon System: Implications for the Detection and Characterization of Earthlike Extrasolar Planets and their Moonlike Companions
- Solar System Physics for Exoplanet Research
- Planet-Planet Occultations in TRAPPIST-1 and Other Exoplanet Systems
- Detectability of extrasolar moons as gravitational microlenses
- How to determine an exomoon's sense of orbital motion
- CHEOPS performance for exomoons: The detectability of exomoons by using optimal decision algorithm
- Some inconvenient truths about biosignatures involving two chemical species on Earth-like exoplanets
- Revisiting the exomoon candidate signal around Kepler-1625b
- Detecting Exomoons Via Doppler Monitoring of Directly Imaged Exoplanets
- Effects of Mutual Transits by Extrasolar Planet-Companion Systems on Light Curves
- On the Detection of Exomoons Transiting Isolated Planetary-Mass Objects
- Predictable patterns in planetary transit timing variations and transit duration variations due to exomoons
- Orbital Stability of Exomoons and Submoons with Applications to Kepler 1625b-I
- Transiting Extrasolar Planet with a Companion: Effects of Orbital Eccentricity and Inclination
- Detecting Exomoons Around Self-luminous Giant Exoplanets Through Polarization
- Extrasolar Binary Planets II: Detectability by Transit Observations
- The Rossiter-McLaughlin effect for exomoons or binary planets
- Catalogue of exoplanets accessible in reflected starlight to the Nancy Grace Roman Space Telescope. A population study and prospects for phase-curve measurements
- Application of Orbital Stability and Tidal Migration Constraints for Exomoon Candidates
- On The Feasibility of Exomoon Detection Via Exoplanet Phase Curve Spectral Contrast
- Large Interferometer For Exoplanets (LIFE). X. Detectability of currently known exoplanets and synergies with future IR/O/UV reflected-starlight imaging missions
- Impact of Tides on the Potential for Exoplanets to Host Exomoons
- First Doppler Limits on Binary Planets and Exomoons in the HR 8799 System
- Analytic Light Curves in Reflected Light: Phase Curves, Occultations, and Non-Lambertian Scattering for Spherical Planets and Moons
- On the Detection of Extrasolar Moons and Rings
- Next Generation of Telescopes or Dynamics Required to Determine if Exo-Moons have Prograde or Retrograde Orbits
- The Exomoon Corridor for Multiple Moon Systems
- Exomoons in Systems with a Strong Perturber: Applications to Cen AB
- Transit Light-curves for Exomoons: Analytical Formalism
- Exploring exomoon atmospheres with an idealized general circulation model
- Traces of exomoons in computed flux and polarization phase curves of starlight reflected by exoplanets
- Tidally Heated Exomoons around Eridani b: Observability and prospects for characterization
- Direct detectability of tidally heated exomoons by photometric orbital modulation
- The "Drake equation" of exomoons -- a cascade of formation, stability and detection
- Updated Studies on Exomoons in the HD 23079 System
- Hot Moons and Cool Stars
- Photobombing Earth 2.0: Diffraction Limit Related Contamination and Uncertainty in Habitable Planet Spectra
- Search for Super Earths by Timing of Transits with CoRoT
- Future Exoplanet Research: Science Questions and How to Address Them
- Exploring Exoplanet Dynamics with JWST: Tides, Rotation, Rings, and Moons
- Possibility for albedo estimation of exomoons: Why should we care about M dwarfs?
- Explicit relations and criteria for eclipses, transits and occultations
- The effect of post-Newtonian spin precessions on the evolution of exomoons' obliquity
- Special cases : moons, rings, comets, trojans
- Enhanced thermal radiation from a tidally heated exomoon with a single hot spot
- Fourier series for eclipses on exoplanet binaries