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Current Members


Interested in joining us? We are always searching for interesting and interested undergraduates, graduate students, and postdocs with a passion for planetary astronomy. Applications for admissions to Caltech as an undergraduate or graduate student (usually in either planetary science or astronomy) are due once a year. Postdoc positions are sometimes posted, though just as frequently postdocs come with external fellowships.

You can view more pictures of the group in action.


Past members

Postdocs

Graduate Students

Undergraduate students

  • Jessica Roberts
  • Christine Chen
  • Sarah Horst (Professor, Johns Hopkins)
  • Dave Tytell
  • Matt Tiscerno


group

p9

Finding Planet Nine

The search for Planet Nine currently involves everything from large scale computer simulation, to meticulous calculation of orbital biases, to large scale surveying with the Subaru telescope, to analysis of massive quantities of archival data in search of already-existing images, to development and refinement of new algorithms to enable all aspects of the search. Things will get even more intense when we actually find it.


h2o2

Exploring the icy satellites of Jupiter

The compositions of the surfaces of the icy satellites of Jupiter are affected by internal processes, such as upwelling from the ocean on Europa or interaction with the magnetic field of Ganymede, and by external forces such as meteorite bomdardment and irradiation from the harsh Jovian magnetospheric environment. We are using Keck Observatory and Hubble Space Telescope spectroscopy to explore these moons and performing laboratory-based experimental work to try to understand what we see.


iab

Uncovering clues to the evolution of the solar system

The small bodies of the outer solar system, from Jupiter Trojan asteroids, to the Centaurs, to the Kuiper belt objects, contain chemical and dynamical clues to the formation and evolution of the solar system. We are engaged in physical studies of these bodies using infrared spectroscopy from the Keck Observatory as well as large-scale population studies using the Subaru Telescope and data from large public surveys to try to read this fossil record.


alma

Detecting heat from bodies in the outer solar system

The ALMA interferometer in Chile has unprecedented spatial resolution and sensitivity. We are mapping thermal emission from Europa, looking for any hot spots potentially caused bu liquid water close to the surface, as well as other thermal anomalies. In addition we are measuring thermal emission from Jupiter Trojan asteroids in search of ice on the surfaces of the smallest of these bodies and searching for emission from distant dwarf planets and their satellites.


Lucy logo

Journeying to the Trojan asteroids with the Lucy mission

Lucy will launch in 2021 en route to the L4 Jupiter Trojan cloud, where, in 2027-28 it will fly by four Trojans, 3548 Eurybates, 15094 Polymele, 11351 Leucus, and 21900 Orus. After these flybys, Lucy will return to the vicinity of the Earth whereupon it will receive a gravity assist to take it to the L5 Trojan cloud (which trails about 60° behind Jupiter), where it will visit the binary Trojan 617 Patroclus with its satellite Menoetius in 2033. Much work is being done by the science team right now to be ready for the first encounter in 2027.


Our group explores the solar system using a wide variety of observational, computation, and experimental facilities.

Keck

The Keck Observatory is our main facility for both high resolution infrared adaptive optics observations and for spectroscopy of faint icy bodies in the outer solar system.



HST

We use Hubble Space Telescope to map the compositions of icy moons and to search for and measure the orbits of satellites of distant solar system objects.




ALMA

The ALMA Observatory in Chile allows us the spatial resolution to obtain images of thermal emission from the Galilean and also has the sensitivity to detect thermal emission from tiny asteroids and distant dwarf planets.


palomar

The 70-yr old 200-inch telescope at Palomar Observatory remains a top-notch astronomical facility. We use it mainly for measuring colors of distant solar system objects.




subaru

The Subaru Telescope, with its massive Hyper-Suprime Cam, is the premiere telescope in the world for survey vast swaths of sky for faint objects. Part of our Planet Nine search is underway there.




HPC

The Caltech High Performance Computer Cluster is critical for running our massive suites of computer simulations in search of Planet Nine.






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Brown Lab

Our new Ice Lab is nearly complete. We now have the capability of obtaining 0.2-20 micron spectra of irradiated Europa analog ices, along with other fun things!