activity
20132021
most citedA Mechanism of Exciting Planetary Inclination and Eccentricity through a Residual Gas Disk

35 citations · 164 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2021★ 18 cited

Non-principal axis rotation in binary asteroid systems and how it weakens the BYORP effect

Alice C. Quillen, Anthony LaBarca, YuanYuan Chen

Using viscoelastic mass/spring model simulations, we explore tidal evolution and migration of compact binary asteroid systems. We find that after the secondary is captured into a s…

astro-ph.EP2018★ 22 cited

Transiting Exoplanet Monitoring Project (TEMP). IV. Refined System Parameters, Transit Timing Variations and Orbital Stability of the Transiting Planetary System HAT-P-25

Xian-Yu Wang, Songhu Wang, Tobias C. Hinse +12

We present eight new light curves of the transiting extra-solar planet HAT-P-25b obtained from 2013 to 2016 with three telescopes at two observatories. We use the new light curves,…

astro-ph.EP2018★ 25 cited

Impact Excitation of a Seismic Pulse and Vibrational Normal Modes on Asteroid Bennu and Associated Slumping of Regolith

Alice C. Quillen, Yuhui Zhao, YuanYuan Chen +3

We consider an impact on an asteroid that is energetic enough to cause resurfacing by seismic reverberation and just below the catastrophic disruption threshold, assuming that seis…

astro-ph.EP2017★ 14 cited

Transiting Exoplanet Monitoring Project (TEMP). III. On the Relocation of the Kepler-9~b Transit

Songhu Wang, Dong-Hong Wu, Brett C. Addison +24

The Kepler-9 system harbors three known transiting planets. The system holds significant interest for several reasons. First, the outer two planets exhibit a period ratio that is c…

astro-ph.EP2017★ 12 cited

Tilting Styx and Nix but not Uranus with a Spin-Precession-Mean-motion resonance

Alice C. Quillen, Yuan-Yuan Chen, Benoit Noyelles +1

A Hamiltonian model is constructed for the spin axis of a planet perturbed by a nearby planet with both planets in orbit about star. We expand the planet-planet gravitational poten…

astro-ph.EP2017★ 31 cited

Obliquity evolution of the minor satellites of Pluto and Charon

Alice C. Quillen, Fiona Nichols-Fleming, Yuan-Yuan Chen +1

New Horizons mission observations show that the small satellites Styx, Nix, Kerberos and Hydra, of the Pluto-Charon system, have not tidally spun-down to near synchronous spin stat…

astro-ph.EP2016★ 6 cited

The effect of orbital damping during planet migration on the Inclination and Eccentricity Distributions of Neptune Trojans

Yuan-Yuan Chen, Yuehua Ma, Jiaqing Zheng

We explore planetary migration scenarios for formation of high inclination Neptune Trojans (NTs) and how they are affected by the planetary migration of Neptune and Uranus. If Nept…

astro-ph.EP2014★ 1 cited

How to reach the orbital configuration of the inner three planets in HD 40307 Planet System ?

Chen Yuan-Yuan, Zhou Ji-Lin, Ma Yue-Hua

The formation of the present configuration of three hot super-Earths in the planet system HD 40307 is a challenge to dynamical astronomers. With the two successive period ratios bo…

astro-ph.EP2013★ 35 cited

A Mechanism of Exciting Planetary Inclination and Eccentricity through a Residual Gas Disk

Yuan-Yuan Chen, Hui-Gen Liu, Gang Zhao +1

Accordling to the theory of Kozai resonance, the initial mutual inclination between a small body and a massive planet in an outer circular orbit is as high as fo…