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PLATO (PLAnetary Transits and Oscillations of stars) is ESA’s M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large number of stars. PLATO will detect small planets (down to
Aerts, Conny+26 more
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Orbital motions and the conservation-law/preferred-frame $\alpha_3$ parameter [PDF]
We analytically calculate some orbital effects induced by the Lorentz-invariance/momentum-conservation PPN parameter $\alpha_3$ in a gravitationally bound binary system made of a compact primary orbited by a test particle.
Iorio, Lorenzo
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The production of proton-rich isotopes beyond iron: The ?-process in stars [PDF]
© 2016 World Scientific Publishing Company. Beyond iron, a small fraction of the total abundances in the Solar System is made of proton-rich isotopes, the p-nuclei.
, , Pignatari, Marco, Travaglio, Claudia
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Absence of a metallicity effect for ultra-short-period planets [PDF]
Ultra-short-period (USP) planets are a newly recognized class of planets with periods shorter than one day and radii smaller than about 2 Earth radii.
Cargile, Phillip+9 more
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EXONEST: The Bayesian Exoplanetary Explorer [PDF]
The fields of astronomy and astrophysics are currently engaged in an unprecedented era of discovery as recent missions have revealed thousands of exoplanets orbiting other stars.
Angerhausen, Daniel+6 more
core +4 more sources
Three Small Planets Transiting a Hyades Star [PDF]
We present the discovery of three small planets transiting K2-136 (LP 358 348, EPIC 247589423), a late K dwarf in the Hyades. The planets have orbital periods of $7.9757 \pm 0.0011$, $17.30681^{+0.00034}_{-0.00036}$, and $25.5715^{+0.0038}_{-0.0040 ...
Albrecht, Simon+35 more
core +4 more sources
Testing Lorentz symmetry with planetary orbital dynamics [PDF]
Planetary ephemerides are a very powerful tool to constrain deviations from the theory of General Relativity using orbital dynamics. The effective field theory framework called the Standard-Model Extension (SME) has been developed in order to ...
Bailey, Quentin G.+8 more
core +4 more sources
The structure of protoplanetary discs around evolving young stars [PDF]
The formation of planets with gaseous envelopes takes place in protoplanetary accretion discs on time-scales of several millions of years. Small dust particles stick to each other to form pebbles, pebbles concentrate in the turbulent flow to form ...
Bitsch, Bertram+3 more
core +1 more source
Analytical expressions for the orbital precessions affecting the relative motion of the components of a local binary system induced by Lorentz-violating Preferred Frame Effects (PFE) are explicitly computed in terms of the PPN parameters $\alpha_1 ...
Iorio, Lorenzo
core +1 more source
Observing Strategies for the Detection of Jupiter Analogs [PDF]
To understand the frequency, and thus the formation and evolution, of planetary systems like our own solar system, it is critical to detect Jupiter-like planets in Jupiter-like orbits.
B. D. Carter+11 more
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