A Closely-Packed System of Low-Mass, Low-Density Planets Transiting Kepler-11
arXiv:1102.0291 · doi:10.1038/nature09760
Abstract
When an extrasolar planet passes in front of its star (transits), its radius can be measured from the decrease in starlight and its orbital period from the time between transits. Multiple planets transiting the same star reveal more: period ratios determine stability and dynamics, mutual gravitational interactions reflect planet masses and orbital shapes, and the fraction of transiting planets observed as multiples has implications for the planarity of planetary systems. But few stars have more than one known transiting planet, and none has more than three. Here we report Kepler spacecraft observations of a single Sun-like star that reveal six transiting planets, five with orbital periods between 10 and 47 days plus a sixth one with a longer period. The five inner planets are among the smallest whose masses and sizes have both been measured, and these measurements imply substantial envelopes of light gases. The degree of coplanarity and proximity of the planetary orbits imply energy dissipation near the end of planet formation.
published in Nature
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- Orbital stability of compact three-planet systems, I: Dependence of system lifetimes on initial orbital separations and longitudes
- A Super-Earth Orbiting Near the Inner Edge of the Habitable Zone around the M4.5-dwarf Ross 508
- Updated Catalog of Kepler Planet Candidates: Focus on Accuracy and Orbital Periods
- APOSTLE: Eleven Transit Observations of TrES-3b
- The origins of nearly coplanar, non-resonant systems of close-in super-Earths
- Planetary Orbital Equations in Externally-Perturbed Systems: Position and Velocity-Dependent Forces
- Planetary Migration in Protoplanetary Disks
- Properties of the single Jovian planet population and the pursuit of Solar system analogues
- Systematic Search for Rings around Kepler Planet Candidates: Constraints on Ring Size and Occurrence Rate
- Predicting Planets in Kepler Multi-Planet Systems
- CoRoT-22 b: a validated 4.9 RE exoplanet in 10-day orbit
- Roche-lobe overflow in eccentric planet-star systems
- Indications for transit timing variations in the exo-Neptune HAT-P-26b
- Consequences of tidal interaction between disks and orbiting protoplanets for the evolution of multi-planet systems with architecture resembling that of Kepler 444
- Planetary Phase Variations of the 55 Cancri System
- Breaking mean-motion resonances during Type I planet migration
- Decoupling Phase Variations in Multi-Planet Systems
- Terrestrial Planets Formation under Migration: the Systems near 4:2:1 Mean Motion Resonance
- Disruption of co-orbital (1:1) planetary resonances during gas-driven orbital migration
- Next Generation of Telescopes or Dynamics Required to Determine if Exo-Moons have Prograde or Retrograde Orbits
- SOPHIE velocimetry of Kepler transit candidates: X KOI-142c: first radial velocity confirmation of a non-transiting exoplanet discovered by transit timing
- Dynamics and Collisional Evolution of Closely Packed Planetary Systems
- Exoplanetary Geophysics -- An Emerging Discipline
- Global Analysis of KOI-977: Spectroscopy, Asteroseismology, and Phase-curve Analysis
- Spitzer Infrared Observations and Independent Validation of the Transiting Super-Earth CoRoT-7b
- The Dynamics of Tightly-packed Planetary Systems in the Presence of an Outer Planet: case studies using Kepler-11 and Kepler-90
- Photodynamical analysis of the nearly resonant planetary system WASP-148: Accurate transit-timing variations and mutual orbital inclination
- Probable Spin-Orbit Aligned Super-Earth Planet Candidate KOI-2138.01
- Resonances of Multiple Exoplanets and Implications for Their Formation
- Signatures of impact-driven atmospheric loss in large ensembles of exoplanets
- In Situ and Ex Situ Formation Models of Kepler 11 Planets
- Forming Different Planetary Systems
- Super-Earths as Failed Cores in Orbital Migration Traps
- Atmospheric Mass Loss from High Velocity Giant Impacts
- ExELS: an exoplanet legacy science proposal for the ESA Euclid mission. II. Hot exoplanets and sub-stellar systems
- Architecture Classification for Extrasolar Planetary Systems
- Conservation of Total Escape from Hydrodynamic Planetary Atmospheres
- Detection of transit timing variations in excess of one hour in the Kepler multi-planet candidate system KOI 806 with the GTC
- Near Mean Motion Resonance of Terrestrial Planet Pair Induced by Giant Planet: Application to Kepler-68 System
- Transits Probabilities Around Hypervelocity and Runaway Stars
- A Pluto--Charon Sonata: Dynamical Limits on the Masses of the Small Satellites
- Methane Planets and their Mass-Radius Relation
- There might be giants: unseen Jupiter-mass planets as sculptors of tightly-packed planetary systems
- A Method to Identify the Boundary Between Rocky and Gaseous Exoplanets from Tidal Theory and Transit Durations
- The Lick-Carnegie Survey: A New Two-Planet System Around the Star HD 207832
- VaTEST I: Validation of Sub-Saturn Exoplanet TOI-181b in Narrow Orbit from its Host Star
- Transiting planets as a precision clock to constrain the time variation of the gravitational constant
- Transit-timing measurements with the model-independent barycenter method: Application to the LHS 6343 system
- Stellar activity and planetary atmosphere evolution in tight binary star systems
- GJ 357 b: A Super-Earth Orbiting an Extremely Inactive Host Star
- The silicate model and carbon rich model of CoRoT-7b, Kepler-9d and Kepler-10b
- Making systems of Super Earths by inward migration of planetary embryos
- Outer Architecture of Kepler-11: Constraints from Coplanarity
- Orbital Dynamics of Exoplanetary Systems Kepler-62, HD 200964 and Kepler-11
- Vetting Kepler Planet Candidates with Multi-Color Photometry from the GTC: Identification of an Eclipsing Binary Star Near KOI 565
- Possible scenarios for eccentricity evolution in the extrasolar planetary system HD 181433
- Orbital stability of compact three-planet systems, II: Post-instability impact behaviour
- exoMMR: a New Python Package to Confirm and Characterize Mean Motion Resonances
- HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS
- Phase Curves of the Kepler-11 Multi-Planet System
- Substructures in protoplanetary disks imprinted by compact planetary systems
- Transit Depth Variations Reveal TOI-216 b to be a Super-Puff
- XUE. JWST spectroscopy of externally irradiated disks around young intermediate-mass stars
- Exploiting the transit timing capabilities of Ariel
- APOSTLE: Longterm Transit Monitoring and Stability Analysis of XO-2b
- TTV Constraints on Additional Planets in the WD 1856+534 system
- In-depth characterization of the Kepler-10 three-planet system with HARPS-N radial velocities and Kepler transit timing variations
- The Habitability of GJ 357 d : Possible Climates and Observability
- Measuring the Orbital Parameters of Radial Velocity Systems in Mean Motion Resonance---a Case Study of HD 200964
- Kepler's Last Planet Discoveries: Two New Planets and One Single-Transit Candidate from K2 Campaign 19
- Null transit detections of 68 radial velocity exoplanets observed by TESS
- Effects of Thermodynamics on the Concurrent Accretion and Migration of Gas Giants in Protoplanetary Disks
- Forecasting the detectability of known radial velocity planets with the upcoming CHEOPS mission
- Combining high-contrast imaging with high-resolution spectroscopy: Actual on-sky MIRI/MRS results compared to expectations
- The architecture of multi-planet systems as a tracer of their formation mechanisms
- The discovery and legacy of Kepler's multi-transiting planetary systems
- The Occurrence-weighted Median Planets Discovered by Transit Surveys Orbiting Solar-type Stars and Their Implications for Planet Formation and Evolution
- Extrasolar enigmas: from disintegrating exoplanets to exoasteroids
- Orbital stability of compact three-planet systems III. The role of three-body resonances
- Dynamical Evolution of Planetary Systems
- Particle dynamics in TOI-178 planetary system
- Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
- TFAW survey II: 6 Newly Validated Planets and 13 Planet Candidates from K2
- Why the dark matter of galaxies is clumps of micro-brown-dwarfs and not Cold Dark Matter
- Do the planets in the HD 34445 system really exist?
- Constraining stellar rotation and planetary atmospheric evolution of a dozen systems hosting sub-Neptunes and super-Earths
- The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246
- Inside-Out Planet Formation: VI. Oligarchic Coagulation of Planetesimals from a Pebble Ring?
- Grain Growth in Escaping Atmospheres: Implications for the Radius Inflation of Super-Puffs
- Accounting for Transit Timing Detectability: Biases in Planetary Radius and Orbital Period