All oral presentation sessions are located in the ballroom of the Four Points Sheraton San Jose Airport
Sunday, April 15 |
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4:00 | DDA Committee Meeting in the Chantilly Boardroom of the Four Points Sheraton San Jose Airport | ||
4:00 | Registration opens at Hangar Bar and Grill, restaurant of the Four Points Sheraton San Jose Airport | ||
Opening Reception |
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6:00 | Food available at the reception until 7:30 | ||
Monday, April 16 |
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8:20 | Seth Jacobson, Matija Cuk, and Matthew Tiscareno | SOC and LOC chairs | Introduction and announcements |
The Astronomer Always Rings Twice |
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8:30 | Phil Nicholson | Cornell University | Stellar occultations by Saturn's rings |
8:45 | Matthew Hedman | University of Idaho | Axisymmetric density waves in Saturn's rings |
9:00 | Maryame El Moutamid | Cornell University | Derivation of the torque associated to tesseral resonances |
9:15 | Robert Chancia | University of Idaho | The structure of Jupiter’s main ring from New Horizons: a comparison with other ring-moon systems |
Party in the Spin Room |
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9:30 | Victor Slabinski | US Naval Observatory | Episodic spin-up and spin-down torque on Earth |
9:45 | Matija Cuk | SETI Institute | Early dynamics of the Moon's core |
Coffee Break and Poster Viewing |
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Pebble in the Sky: Meteoroids and Their Orbits |
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10:30 | Althea Moorhead | NASA Marshall Space Flight Center | The formation and early evolution of meteoroid streams (Invited) |
11:00 | Luke Dones | Southwest Research Institute | Asteroids and meteorites from Venus? Only the Earth goddess knows |
11:15 | Margaret Campbell-Brown | University of Western Ontario | Meteoroid orbits from observations (Invited) |
11:45 | Peter Jenniskens | SETI Institute | A shower look-up table to trace the dynamics of meteoroid streams and their sources |
12:00 | Sigrid Close | Stanford University | Electromagnetic effects from impacts on spacecraft (Invited) |
Lunch break |
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'N Sync |
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2:00 | Brett Gladman | University of British Columbia | The prevalence of resonances among large-a trans-Neptunian objects |
2:15 | Kathryn Volk | University of Arizona | Two objects in Neptune's 9:1 resonance -- implications for resonance sticking in the scattering population |
2:30 | Lei Lan | University of Arizona | Neptune's 5:2 mean motion resonance in the Kuiper belt |
2:45 | Thomas Rimlinger | University of Maryland | The stability of resonant chains of moons |
3:00 | Yukun Huang | Tsinghua University | Dynamics of the retrograde 1:1 mean motion resonance |
3:15 | Paul Wiegert | University of Western Ontario | The first retrograde Trojan asteroid |
3:30 | Alex Davis | University of Colorado | Full two-body problem mass parameter observability explored through doubly synchronous systems |
Coffee break and poster viewing |
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The Fault in Our Stars |
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4:15 | Monica Valluri | University of Michigan | Estimating biases in the stellar dynamical black hole mass measurements in barred galaxies and prospects for measuring SMBH masses with JWST |
4:30 | Heather Wernke | University of Colorado | Tidal disruption events from eccentric nuclear disks |
4:45 | Rosemary Wyse | Johns Hopkins University | Stellar angular momentum distributions and preferential Radial Migration |
5:00 | Jing Luan | University of California at Berkeley | DAVs: red edge and outbursts |
5:15 | Kevin Rauch | University of Maryland | HNbody: a simulation package for hierarchical N-body systems |
Public Lecture: Extreme Solar Systems |
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Tuesday, April 17 |
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8:00 | Registration opens | ||
8:20 | Seth Jacobson, Matija Cuk, and Matthew Tiscareno | SOC and LOC chairs | Announcements |
Vera Rubin Prize Lecture |
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8:30 | Dan Fabrycky | University of Chicago | The realm of close-in planets |
Hot, Flat, and Crowded |
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9:15 | Sam Hadden | Harvard University | A resonance overlap criterion for the onset of chaos in systems of two eccentric planets |
9:30 | Daniel Tamayo | University of Toronto at Scarborough | Predicting instability timescales in closely-packed planetary systems |
9:45 | Aaron Boley | University of British Columbia | Transit duration variations due to secular interactions in systems with tightly-packed inner planets |
Coffee Break and Poster Viewing |
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An Oblique Reference to Pop Culture |
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10:30 | Kassandra Anderson | Cornell University | Teetering stars: resonant excitation of stellar obliquities by hot and warm Jupiters with external companions |
10:50 | Christopher Spalding | California Institute of Technology | The resilience of Kepler multi-systems to stellar obliquity |
11:05 | Sarah Millholland | Yale University | On the obliquities of planets in close-in, compact systems |
11:25 | Daniel Jontof-Hutter | University of the Pacific | Dynamical constraints on non-transiting planets at Trappist-1 |
11:40 | Elizabeth Bailey | California Institute of Technology | Probing the parameters of the HAT-P-2 system |
12:00 | David Fleming | University of Washington | On the lack of circumbinary planets orbiting isolated binary stars |
12:15 | Agueda Granados Contreras | University of British Columbia | The formation of co-orbital planets and their resulting transit signatures |
Lunch break |
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In the Beginning There Was Chaos |
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2:00 | Juliette Becker | University of Michigan | Forming hot Jupiters: observational constraints on gas giant formation and migration |
2:15 | Masahiro Ogihara | National Astronomical Observatory of Japan | Formation of close-in super-Earths in an evolving disk due to disk winds |
2:30 | Mickey Rosenthal | University of California at Santa Cruz | How turbulence can set the radial distribution of gas giants formed by pebble accretion |
2:45 | Spencer Wallace | University of Washington | High resolution N-body simulations of terrestrial planet growth |
3:00 | Matthew Clement | University of Oklahoma | Saving the inner solar system with an early instability |
3:15 | Rogerio Deienno | Southwest Research Institute | Exciting an initially cold asteroid belt through a planetary instability |
3:30 | Renata Frelikh | University of California at Santa Cruz | Dynamical upheaval in ice giant formation: a solution to the fine-tuning problem in the formation story |
3:45 | Yu-Cian Hong | Cornell University | Orbital dynamics of exomoons during planet–planet scattering |
Coffee Break and Poster Viewing |
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Lick Observatory Tour |
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Wednesday, April 18 |
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8:00 | Registration opens | ||
8:20 | Seth Jacobson, Matija Cuk, and Matthew Tiscareno | SOC and LOC chairs | Announcements |
Stability, or Instability, That is the Question |
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8:30 | Sacha Gavino | University of Bordeaux | Orbital stability of compact three-planets systems |
8:45 | Fred Adams | University of Michigan | The stability of tidal equilibrium for hierarchical star-planet-moon systems |
9:00 | Pierre Gratia | Northwestern University |
Stability considerations of packed multi-planet systems |
9:15 | Jack Lissauer | NASA Ames Research Center | Stability of multi-planet systems orbiting in the Alpha Centauri AB system |
9:30 | Billy Quarles | University of Oklahoma | Dynamics of circumbinary planets near the stability limit |
9:45 | Alexander Zderic | University of Colorado | Instability timescale for the inclination instability in the solar system |
Coffee Break and Poster Viewing |
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1I/`Oumuamua: the First Known Interstellar Asteroid |
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10:30 | Karen Meech | University of Hawaii | Observations of 1I/`Oumuamua (Invited) |
11:00 | Darryl Seligman | Yale University | The feasibility and benefits of in situ exploration of 1I/`Oumuamua-like objects |
11:15 | Quan-Zhi Ye | California Institute of Technology | Telescopic and meteor observation of 1I/`Oumuamua, the first known interstellar asteroid (Invited) |
11:45 | Daniel Scheeres | University of Colorado | Stability limits for rubble pile asteroid shapes |
12:00 | Darin Ragozzine | Brigham Young University | On the detectability of interstellar objects like 1I/'Oumuamua (Invited) |
Lunch break |
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The Good, the Bad, the Ugly: How Do Simulations Compare Their Data to Observers and How Can They Do It Better? |
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2:00 | Nathan Kaib | University of Oklahoma | Using real and simulated TNOs to constrain the outer solar system (Invited) |
2:30 | Robyn Sanderson | California Institute of Technology | Science with synthetic stellar surveys (Invited) |
3:00 | Kelly Holley-Bockelmann | Vanderbilt University | Supermassive black holes as revealed by LISA: how gravitational wave astronomy will be a game changer (Invited) |
Coffee Break and Poster Viewing |
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Stretched Out Dwarfs |
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4:00 | Cristobal Petrovich | Canadian Institute for Theoretical Astrophysics | Merging black holes in non-spherical nuclear star clusters |
4:15 | Heidi Newberg | Rensselaer Polytechnic Institute | Reconstructing the dwarf galaxy progenitor from tidal streams using MilkyWay@Home |
4:30 | Andrew Wetzel | University of California at Davis | Implications of stellar feedback for dynamical modeling of the Milky Way and dwarf galaxies |
Dirk Brouwer Award Lecture |
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4:45 | Ortwin Gerhard | Max Planck Institute for Extraterrestrial Physics | The barred inner region of the Milky Way |
DDA Member's Annual Meeting |
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Conference Banquet |
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Thursday, April 19 |
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8:00 | Registration opens | ||
8:20 | Seth Jacobson, Matija Cuk, and Matthew Tiscareno | SOC and LOC chairs | Announcements |
Flat Cats Instead of Spherical Cows |
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8:30 | Konstantin Batygin | California Institute of Technology | Schrödinger evolution of self-gravitating disks |
8:45 | Diana Powell | University of California at Santa Cruz | Using ice and dust lines to constrain the surface densities of protoplanetary disks |
9:00 | Wing-Kit Lee | Northwestern University | Long-lived eccentric modes in protoplanetary disks |
9:15 | Andrew Shannon | Pennsylvania State University | The dynamical imprint of lost protoplanets on the trans-Neptunian populations, and limits on the primordial size distribution of trans-Neptunian objects at Pluto and larger sizes. |
9:30 | Joseph A'Hearn | University of Idaho | Dynamics of multiple bodies in a corotation resonance |
Danger, Will Robinson! Danger! |
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9:45 | Alan Harris | MoreData! | NEA impactors: what direction do they come from? |
10:00 | Douglas Hamilton | University of Maryland | Deadly sunflower orbits |
10:15 | Aaron Rosengren | University of Arizona | Chaotic Transport in Circumterrestrial Orbits |
Coffee Break and Poster Viewing |
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Ringleaders and Fellow Travelers |
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11:00 | Marina Brozovic | NASA Jet Propulsion Laboratory | Orbits of the inner satellites of Neptune |
11:15 | Valery Lainey | NASA Jet Propulsion Laboratory | Interior properties of the inner Saturnian moons from space astrometry data |
11:30 | William Oldroyd | Brigham Young University | More sophisticated fits of the orbits of Haumea's interacting moons |
Never Tell Me the Odds |
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11:45 | Benjamin Proudfoot | Brigham Young University | Modeling the dynamical structure of the Haumea family |
12:00 | Nathan Benfell | Brigham Young University | Assessing backwards integration as a method of KBO family finding |
12:15 | Tali Khain | University of Michigan | The generation of the distant Kuiper belt by planet nine from an initially broad perihelion distribution |
12:35 | Steven Maggard | Brigham Young University | Dynamical classifications of the Kuiper belt |
12:50 | Christa Van Laerhoven | University of British Columbia | Determining the plane of the Kuiper belt with OSSOS |
All poster presentation sessions are located in the back section of the ballroom of the Four Points Sheraton San Jose Airport
Available all week |
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1 | Aaron Boley | The University of British Columbia | The sustainable development of space: astro-environmental and dynamical considerations |
2 | Michael Cahill | University of Wisconsin-Washington County | Cellular analysis of boltzmann most probable ideal gas statistics |
3 | Rogerio Deienno | Southwest Research Institute | Terrestrial planet formation from an annulus -- revisited |
4 | David Fleming | University of Washington | Coevolution of binaries and circumbinary gaseous disks |
5 | Robert Jacobson | Jet Propulsion Laboratory | Constraints on the mass and location of planet 9 set by range and VLBI observations of Cassini |
6 | Seth Jacobson | Northwestern University | Planetary cross-breeding: geochemical mixing during planet formation |
7 | Satish Malhotra | Gravity does it: redshift of light from the galaxies yes, expanding universe no! | |
8 | Chris Mankovich | University of California at Santa Cruz | A View into Saturn through its Natural Seismograph |
9 | William Polycarpe | IMCCE | Titan crossing a 5:1 MMR with Iapetus: constraining the tidal recession of Titan and giving an explanation for Iapetus' current orbit |
10 | Zeeve Rogoszinski | University of Maryland | Supermassive black holes as revealed by LISA: how gravitational wave astronomy will be a game changer |
11 | Chris Simonson | High-velocity cloud complex h and Weaver’s “jet”: two candidate dwarf satellite galaxies for which dark matter halo models indicate distances of ~27 kpc and ~108 kpc | |
12 | Spencer Wallace | University of Washington | The influence of dynamical friction and mean motion resonances on terrestrial planet growth |