Stellar obliquities in exoplanetary systems

SH Albrecht, RI Dawson, JN Winn - Publications of the …, 2022 - iopscience.iop.org
The rotation of a star and the revolutions of its planets are not necessarily aligned. This
article reviews the measurement techniques, key findings, and theoretical interpretations …

The planet nine hypothesis

K Batygin, FC Adams, ME Brown, JC Becker - Physics Reports, 2019 - Elsevier
Over the course of the past two decades, observational surveys have unveiled the intricate
orbital structure of the Kuiper Belt, a field of icy bodies orbiting the Sun beyond Neptune. In …

The imprint of exoplanet formation history on observable present-day spectra of hot Jupiters

C Mordasini, R van Boekel, P Mollière… - The Astrophysical …, 2016 - iopscience.iop.org
The composition of a planet's atmosphere is determined by its formation, evolution, and
present-day insolation. A planet's spectrum therefore may hold clues on its origins. We …

Free-floating Planet Mass Function from MOA-II 9 yr Survey toward the Galactic Bulge

T Sumi, N Koshimoto, DP Bennett… - The Astronomical …, 2023 - iopscience.iop.org
We present the first measurement of the mass function of free-floating planets (FFPs), or very
wide orbit planets down to an Earth mass, from the MOA-II microlensing survey in 2006 …

Predictions of the nancy grace roman space telescope galactic exoplanet survey. II. Free-floating planet detection rates

SA Johnson, M Penny, BS Gaudi, E Kerins… - The Astronomical …, 2020 - iopscience.iop.org
Abstract The Nancy Grace Roman Space Telescope (Roman) will perform a Galactic
Exoplanet Survey (RGES) to discover bound exoplanets with semimajor axes greater than 1 …

Close encounters: How stellar flybys shape planet-forming discs

N Cuello, F Ménard, DJ Price - The European Physical Journal Plus, 2023 - Springer
We review the role of stellar flybys and encounters in shaping planet-forming discs around
young stars, based on the published literature on this topic in the last 30 years. Since most …

A giant exoplanet orbiting a very-low-mass star challenges planet formation models

JC Morales, AJ Mustill, I Ribas, MB Davies, A Reiners… - Science, 2019 - science.org
Surveys have shown that super-Earth and Neptune-mass exoplanets are more frequent than
gas giants around low-mass stars, as predicted by the core accretion theory of planet …

Stellar clustering shapes the architecture of planetary systems

AJ Winter, JMD Kruijssen, SN Longmore, M Chevance - Nature, 2020 - nature.com
Planet formation is generally described in terms of a system containing the host star and a
protoplanetary disk,–, of which the internal properties (for example, mass and metallicity) …

Characterization of exoplanets from their formation-i. models of combined planet formation and evolution

C Mordasini, Y Alibert, H Klahr, T Henning - Astronomy & Astrophysics, 2012 - aanda.org
Context. A first characterization of extrasolar planets by the observational determination of
the radius has recently been achieved for a large number of planets. For some planets, a …

Characterization of exoplanets from their formation-II. The planetary mass-radius relationship

C Mordasini, Y Alibert, C Georgy, KM Dittkrist… - Astronomy & …, 2012 - aanda.org
Context. The research of extrasolar planets has entered an era in which we characterize
extrasolar planets. This has become possible with measurements of the radii of transiting …