The Remote Sensing Observers Group aims to increase scientific knowledge of all Solar System bodies by serving as a center of experts in the operation and development of remote sensing instruments and analysis tools, leveraging all possible ground- and space-based assets.

Selected Projects

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Europa Clipper

NASA's Europa Clipper will conduct detailed reconnaissance of Jupiter's moon Europa and investigate whether the icy moon could harbor conditions suitable for life. The Europa Ultraviolet Imaging Spectrograph (Europa-UVS) is considered the “plume hunter” for the mission, and will study Europa’s atmosphere, environment, and surface. This instrument is being built at the Southwest Research Institute, with significant involvement from the RSO group.

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Juno

Juno is a solar-powered NASA funded spacecraft, which inserted into polar elliptical orbit around Jupiter on July 4 2016. Juno is designed to answer the following science questions: (1) how is Jupiter structured on the inside; (2) how did Jupiter form and shape the solar system formation; (3) how does Jupiter’s atmospheric structure and dynamics below the cloud tops work; (4) how does Jupiter polar magnetosphere work?

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Lunar Reconnaissance Orbiter

The Lunar Reconnaissance Orbiter is a NASA robotic spacecraft currently orbiting the Moon in an eccentric polar mapping orbit. Data collected by LRO have been described as essential for planning NASA's future human and robotic missions to the Moon.

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New Horizons

New Horizons is an interplanetary space probe that was launched as a part of NASA's New Frontiers program in 2006 with the primary mission to perform a flyby study of the Pluto system in 2015, and a secondary mission to fly by and study one or more other Kuiper belt objects (KBOs).

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TEXES

TEXES is a high-resolution mid-infrared spectrograph that has been a regular visitor instrument at NASA’s Infrared Telescope Facility and the Gemini North telescope for the last twenty years. During this time, it has been used to observe a wide range of targets, from star forming regions to planets and moons in the solar system. The high spectral resolution (R=80,000) capabilities of the instrument allow molecular absorption/emission lines to be spectrally separated, while the TEXES scan-map mode means that spectral image cubes can be built up for extended objects.

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JUICE

JUICE is a European Space Agency mission launching in 2022, with the goal of characterizing Jupiter’s three icy moons – Europa, Ganymede and Callisto. These moons are of particular scientific interest as they are considered to be among the most potentially habitable places in the solar system. The mission will also study Jupiter itself, providing new insights into the ways in which gas giant planets form and evolve. JUICE will reach the Jupiter system in 2029 and will perform a series of flybys of the icy moons before entering into orbit around Ganymede, becoming the first spacecraft to orbit any solar system moon other than our own.

Meet Our Team

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Anicia Arredondo

Infrared spectroscopy, small body surfaces, and volatiles in the solar system.

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Tracy Becker

UV spectroscopy, planetary ring occultations, radar observations of asteroids.

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Cesare Grava

Modeling of volatile transport in and spectroscopic observations of airless bodies in the Solar System.

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Thomas Greathouse

UV, IR instrument development, observations of gas planets, atmospheric models.

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Rohini Giles

Infrared observations, radiative transfer modeling of atmospheres.

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Stephanie Jarmak

Planetary ring occultations, ground-based and flight-based microgravity experiments, development of CubeSat missions.

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Josh Kammer

UV spectroscopy and solar/stellar occultations by planetary atmospheres.

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Pippa Molyneux

UV spectroscopy of planetary atmospheres and surfaces; UV instrumentation.