papers

Publications (9)

astro-ph.EP2022

Anticipating the DART impact: Orbit estimation of Dimorphos using a simplified model

Shantanu P. Naidu, Steven R. Chesley, Davide Farnocchia +5

We used the times of occultations and eclipses between the components of the 65803 Didymos binary system observed in its lightcurves from 2003-2021 to estimate the orbital paramete…

astro-ph.EP2015

Sublimation-Driven Activity in Main-Belt Comet 313P/Gibbs

Henry H. Hsieh, Olivier Hainaut, Bojan Novakovic +15

We present an observational and dynamical study of newly discovered main-belt comet 313P/Gibbs. We find that the object is clearly active both in observations obtained in 2014 and…

astro-ph.EP2024

Properties of outer solar system pebbles during planetesimal formation from meteor observations

Peter Jenniskens, Paul R. Estrada, Stuart Pilorz +42

In the late stages of accretion leading up to the formation of planetesimals, particles grew to pebbles the size of 1-mm to tens of cm. That is the same size range that dominates t…

astro-ph.EP2026

Unmasking (44) Nysa: Evidence for a trilobate structure

Kate Minker, Anthony Berdeu, Gianluca Li Causi +16

Context. (44) Nysa is one of the largest known E-type asteroids. Light curve inversion models have indicated that it may have an elongated shape commonly found in large binary syst…

astro-ph.EP2026

Dynamic Trajectory Analysis of Meteoroids Showing Minimal Deceleration

Thomas Stevenson, Ellie Sansom, Hadrien Devillepoix +8

Meteoroids decelerate and ablate as they descend through the atmosphere, however a portion of instrumentally observed meteors show little measurable deceleration and remain poorly…

astro-ph2006

No Detectable H3+ Emission from the Atmospheres of Hot Jupiters

Evgenya Shkolnik, Eric Gaidos, Nick Moskovitz

H emission is the dominant cooling mechanism in Jupiter's thermosphere and a useful probe of temperature and ion densities. The H ion is predicted to form in the thermo…