Interstellar Updates

Laser Propulsion Science and Technology
https://www.mdpi.com/2226-4310/11/10/806

Assessment of Ensemble-Based Machine Learning Algorithms for Exoplanet Identification
https://www.mdpi.com/2079-9292/13/19/3950

Interpretation of the Transit Light Curve in the Presence of Principal Main Minimum with Allowance for the Eccentricity of the Transit (Planet) Orbit
https://link.springer.com/article/10.1134/S1063772924700598

Searching for small primordial black holes in planets, asteroids and here on Earth
https://www.sciencedirect.com/science/article/abs/pii/S2212686424002449

Gas dynamics around a Jupiter-mass planet – I. Influence of protoplanetary disk properties
https://www.aanda.org/articles/aa/full_html/2024/10/aa50899-24/aa50899-24.html

JWST reveals the rapid and strong day-side variability of 55 Cancri e
https://www.aanda.org/articles/aa/full_html/2024/10/aa50748-24/aa50748-24.html

Partial Disruption of a Planet around a White Dwarf: The Effect of Perturbations from the Remnant Planet on the Accretion
https://iopscience.iop.org/article/10.3847/1538-4357/ad73d3

Lava Worlds Surface Measurements at High Temperatures
https://iopscience.iop.org/article/10.3847/2041-8213/ad7d89

Gen TSO: A General JWST Simulator for Exoplanet Times-series Observations
https://arxiv.org/abs/2410.04856

The Search for Disk Perturbing Planets Around the Asymmetrical Debris Disk System HD 111520 Using REBOUND
https://arxiv.org/abs/2410.03932

Breaking degeneracies in exoplanetary parameters through self-consistent atmosphere-interior modelling
https://arxiv.org/abs/2410.04470

Constraining Planetary Albedo of JWST Targets in the TESS bandpass, using TESS, HST and Spitzer Eclipse Depth Observations
https://arxiv.org/abs/2410.04804

SETI in 2022
https://www.sciencedirect.com/science/article/abs/pii/S0094576524005745

Planet found in star’s ‘forbidden zone’
https://www.sciencedirect.com/science/article/abs/pii/S026240792401772X

On the origin of transition disk cavities: Pebble-accreting protoplanets vs Super-Jupiters
https://arxiv.org/abs/2410.02856

Constraining the Presence of Companion Planets in Hot Jupiter Planetary System Using TTV Observation from TESS
https://arxiv.org/abs/2410.03101

sunset: A database of synthetic atmospheric-escape transmission spectra for nearly every transiting planet
https://arxiv.org/abs/2410.03228

A General, Differentiable Transit Model for Ellipsoidal Occulters: Derivation, Application, and Forecast of Planetary Oblateness and Obliquity Constraints with JWST
https://arxiv.org/abs/2410.03449

The Feasibility of Asynchronous Rotation via Thermal Tides for Diverse Atmospheric Compositions
https://arxiv.org/abs/2410.03491

JWST/NIRISS reveals the water-rich “steam world” atmosphere of GJ 9827 d
https://arxiv.org/abs/2410.03527

Microscopic Coherent Sources of Gravitational Radiation with Application to Forming a Stable Warp Field
https://www.preprints.org/manuscript/202409.2370/v1

Structural evolution of liquid silicates under conditions in Super-Earth interiors
https://www.nature.com/articles/s41467-024-51796-7

The social science perspective on the Fermi paradox
https://www.cambridge.org/core/journals/international-journal-of-astrobiology/article/social-science-perspective-on-the-fermi-paradox/449E3C7859EEB602974F25B3E1481E03

Ejected from home: C/1980 E1 (Bowell) and C/2024 L5 (ATLAS)
https://arxiv.org/abs/2410.01975

TESS Asteroseismic Masses and Radii of Red Giants with (and without) Planets
https://arxiv.org/abs/2410.02051

Evidence that Planets in the Radius Gap Do Not Resemble Their Neighbors
https://arxiv.org/abs/2410.02150

Polarized Signatures of the Earth Through Time: An Outlook for the Habitable Worlds Observatory
https://arxiv.org/abs/2410.02194

BEBOP VI. Enabling the detection of circumbinary planets orbiting double-lined binaries with the DOLBY method of radial-velocity extraction
https://arxiv.org/abs/2410.02573

Leaning Sideways: VHS 1256-1257 b is a Super-Jupiter with a Uranus-like Obliquity
https://arxiv.org/abs/2410.02672

What doesn’t kill Gaia makes her stronger
https://arxiv.org/abs/2405.05091

Volatile composition of the HD 169142 disk and its embedded planet
https://arxiv.org/abs/2410.01418

Optical design options for Pollux: UV spectropolarimeter project for the Habitable Worlds Observatory
https://arxiv.org/abs/2410.01491

Generating X-ray transit profiles with batman
https://arxiv.org/abs/2410.01559

A Fourth Planet in the Kepler-51 System Revealed by Transit Timing Variations
https://arxiv.org/abs/2410.01625

Self-consistent N-body simulation of Planetesimal-Driven Migration I. The trajectories of single planets in the uniform background
https://arxiv.org/abs/2405.07279

HATS-38 b and WASP-139 b Join a Growing Group of Hot Neptunes on Polar Orbits
https://iopscience.iop.org/article/10.3847/1538-3881/ad70b8

Nightside Clouds on Tidally Locked Terrestrial Planets Mimic Atmosphere-free Scenarios
https://iopscience.iop.org/article/10.3847/2041-8213/ad78de

HZ_evolution: A Package to Calculate Habitable Histories
https://iopscience.iop.org/article/10.3847/2515-5172/ad8129

Promise and Peril: Stellar Contamination and Strict Limits on the Atmosphere Composition of TRAPPIST-1c from JWST NIRISS Transmission Spectra
https://arxiv.org/abs/2409.19333

A sub-Earth-mass planet orbiting Barnard’s star: No evidence of transits in TESS photometry
https://arxiv.org/abs/2410.00577

The Dynamical History of HIP-41378 f — Oblique Exorings Masquerading as a Puffy Planet
https://arxiv.org/abs/2410.00641

Tidal evolution of Earth-like planets in the habitable zone of low-mass stars
https://arxiv.org/abs/2410.00739

The obliquity and atmosphere of the hot Jupiter WASP-122b (KELT-14b) with ESPRESSO: An aligned orbit and no sign of atomic or molecular absorption
https://arxiv.org/abs/2410.00800

Rate-induced biosphere collapse in the Daisyworld model
https://arxiv.org/abs/2410.00043

Promise and Peril: Stellar Contamination and Strict Limits on the Atmosphere Composition of TRAPPIST-1c from JWST NIRISS Transmission Spectra
https://arxiv.org/abs/2409.19333

The Compositions of Rocky Planets in Close-in Orbits Tend to be Earth-Like
https://arxiv.org/abs/2410.00213