planetary systems

Kepler-68: Three Planets, One with a Density between that of Earth and Ice Giants

Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data

On the Relative Sizes of Planets within Kepler Multiple-candidate Systems

The Discovery of HD 37605c and a Dispositive Null Detection of Transits of HD 37605b

Constraining the false positive rate for Kepler planet candidates with multicolour photometry from the GTC

Transit Timing Observations from Kepler. V. Transit Timing Variation Candidates in the First Sixteen Months from Polynomial Models

Out of hundreds of candidate planetary systems, scientists had previously verified six systems with multiple transiting planets. Now, Kepler observations have verified planets in 11 new planetary systems. Many of these systems contain additional planet candidates that are yet to be verified.

Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Interactions between Moderate- and Long-period Giant Planets: Scattering Experiments for Systems in Isolation and with Stellar Flybys

Almost All of Kepler's Multiple-planet Candidates Are Planets

See also papers II , III & IV that led up to this paper. Press Coverage NASA mission piles on the planets: MSNBC, January 26, 2012 [w/ video] NASA's Keplar Spacecraft Finds 11 New Solar Systems, 26 Planets: Mashable, January 27, 2012 [video] Planet-hunting space telescope nets jackpot: January 27, 2012 Kepler uncovers planetary menagerie: Nature News Blog, Janary 27, 2012 La nave Kepler descubre 26 nuevos planetas orbitando en torno a 11 estrellas: El Munod, January 27, 2012 (spanish) NASA Telescope Discovers 26 Alien Planets Around 11 Different Stars: Space.

Constraining the Planetary System of Fomalhaut Using High-resolution ALMA Observations

Zooming in on Fomalhaut This video sequence starts with a wide-field view of the sky around the star Fomalhaut in the constellation of Piscis Austrinus (The Southern Fish). Fomalhaut is the brightest star in the constellation and one of the brightest stars known to have an orbiting planet. It lies about 25 light-years from the Earth and is surrounded by a huge disc of dust. The final view of this video shows a new ALMA image of the disc (orange) and the new results from ALMA have given astronomers a major breakthrough in understanding a nearby planetary system and provided valuable clues about how such systems form and evolve.

Transit Timing Observations from Kepler. II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

Planets in Systems from NASA’s Kepler Mission The image above depicts multiple planet systems discovered by NASA’s Kepler mission and confirmed by transit timing variations (as of January 2012). Out of hundreds of candidate planetary systems, scientists had previously verified six systems with multiple transiting planets (denoted here in red). Now, Kepler observations have verified planets (shown here in green) in 11 new planetary systems. Many of these systems contain additional planet candidates that are yet to be verified (shown here in dark purple).

Transit Timing Observations from Kepler. IV. Confirmation of Four Multiple-planet Systems by Simple Physical Models

Planets in Systems from NASA’s Kepler Mission The image above depicts multiple planet systems discovered by NASA’s Kepler mission and confirmed by transit timing variations (as of January 2012). Out of hundreds of candidate planetary systems, scientists had previously verified six systems with multiple transiting planets (denoted here in red). Now, Kepler observations have verified planets (shown here in green) in 11 new planetary systems. Many of these systems contain additional planet candidates that are yet to be verified (shown here in dark purple).

Kepler-20: A Sun-like Star with Three Sub-Neptune Exoplanets and Two Earth-size Candidates

Kepler-22b: A 2.4 Earth-radius Planet in the Habitable Zone of a Sun-like Star

Probing potassium in the atmosphere of HD 80606b with tunable filter transit spectrophotometry from the Gran Telescopio Canarias

When an exoplanet transits across the face of its host star atoms and gases in its atmosphere absorb some of the starlight at specific wavelengths. These absorption wavelengths form a unique fingerprint, allowing researchers to identify the presence of Potassium.

The Kepler-19 System: A Transiting 2.2 R $_⊕$ Planet and a Second Planet Detected via Transit Timing Variations

Press Coverage Hidden Worlds: Astronomers Find Invisible Planet 650 Light-Years Away: Time, September 9, 2011. Astronomers Discover 'Invisible' Planet With New Technique: International Business Times, September 9, 2011. Transit planet search reveals doubly-tilted solar sytem: USA Today, September 9, 2011. NASA's Kepler spacecraft finds "invisible world": Digital Journal.com, September 8, 2011. "Invisible" planet discovered with new technique: Kepler probe detects alien world by its gravitational influence on a neighbor: MSNBC.

Architecture and Dynamics of Kepler's Candidate Multiple Transiting Planet Systems

Kepler-14b: A Massive Hot Jupiter Transiting an F Star in a Close Visual Binary

Kepler-15b: A Hot Jupiter Enriched in Heavy Elements and the First Kepler Mission Planet Confirmed with the Hobby-Eberly Telescope

Kepler-18b, c, and d: A System of Three Planets Confirmed by Transit Timing Variations, Light Curve Validation, Warm-Spitzer Photometry, and Radial Velocity Measurements