Solar System Studies
Lowell astronomers carry out a wide diversity of research programs with goals tied to understanding the nature, formation, habitability, and evolution of planetary bodies in our solar system.
This work continues the observatory’s legacy of solar system studies. which began with questions about our solar system and our place within it. Founder Percival Lowell established the observatory in 1894 to study the planet Mars at a favorable opposition, and later in 1930 the planet Pluto was discovered by Clyde Tombaugh at the observatory. From those groundbreaking initial studies, planetary research continues at Lowell Observatory.
Modern-day research involves key contributions to ongoing spacecraft missions, performing novel laboratory experiments, and analyzing observations from state-of-the-art ground and space-based telescopes.
Saturn’s rings sport a varied nature, as seen in these images taken by the Cassini spacecraft. The B ring is optically thick and bright, while the F ring (inset) is narrow and tenuous. It also is inclined with respect to Saturn’s equator plane and the other rings. [Source: https://www.sciencemag.org/news/2015/08/satellite-smashup-created-saturns-narrow-f-ring]
Rings around planets and centaurs
Dr. Amanda Bosh studies Centaurs, small bodies that have been scattered inward from the Kuiper Belt region and will eventually either leave the solar system or become Jupiter-family comets. They largely retain the volatile inventory from the time of solar system formation, making them interesting targets of study as windows into the early age of our planetary system. She searches for signs of activity in these bodies, and discovered that Chiron, the first-identified Centaur, has a tenous ring system. She also uses the stellar occultation technique to study the long-term variability of Pluto’s atmosphere and the kinematics of the Saturnian and Uranian ring systems.
Learn more about Dr. Amanda Bosh
Kuiper Belt Object Arrokoth was visited by the New Horizons spacecraft in 2019. The double-lobed shape was suggested by previous stellar occultation data and confirmed during the flyby. [Source: https://www.nasa.gov/feature/far-far-away-in-the-sky-new-horizons-kuiper-belt-flyby-object-officially-named-arrokoth]
Occultations
Dr. Larry Wasserman studies solar system bodies via occultations. His work on occultations includes the prediction, observation, and analysis of data from such events. These observations lead to an understanding of the size and shape of small bodies, parameters that are impossible to determine without an expensive in situ space mission. They can also reveal the presence of an atmosphere, as occurred with Pluto in 1988.
Learn more about Dr. Larry Wasserman
Comet 41P/Tuttle-Giacobini-Kresak displays dramatic jet activity, outflows of gas and dust from the comet’s nucleus. During a six-week period in 2017, this comet’s rotation period slowed by a factor of two. [Source: https://astroengine.com/2017/10/19/spinning-comet-slams-its-brakes-as-it-makes-earth-flyby/]
Comet evolution and rotation
Dr. Dave Schleicher’s major research interests include the physical properties, chemical composition, and behavior of comets. He uses a variety of observational tools plus theoretical modeling in his studies. In 1986, he discovered with Dr. Robert Millis the periodic variability of Comet Halley — a discovery that profoundly affected the interpretation of all observations of the comet including those from the Giotto and Vega craft.
Learn more about Dr. Dave Schleicher
In 2016, data from Nick Moskovitz’s LOCAMS meteorite detection network was used to locate the fall site of a bright fireball observed by more than 400 people. These 12 of the recovered fragments from the Dishchii’bikoh meteorite. [Source: https://azdailysun.com/opinion/columnists/view-from-mars-hill-detecting-an-intruder-from-outer-space/article_cae08725-6a90-5cb7-a2d7-b05ad54cd580.html
Asteroid formation and evolution
Dr. Nick Moskovitz’s research focuses on minor planets in the solar system. His work has implications for topics ranging from the origin of planets to the exploration of small bodies by spacecraft. Topics that Moskovitz and his collaborators are pursing include understanding the link between asteroids and meteorites, characterizing the properties of meteors, probing the geologic evolution of minor planets over solar system history, developing tools to enable mining of minor planet data, and using telescopic observations to support spacecraft missions.
In 2016, data from Nick Moskovitz’s LO-CAMS meteor camera network was used to help locate meteorites from a bright fireball observed by more than 400 people. These are 12 of the recovered fragments from the Dishchii’bikoh meteorite.
Learn more about Dr. Nick Moskovitz
Trans-Neptunian Object 2004 TT357, approximately 150 km in diameter, sports a light curve that is consistent with a two-lobed body. [Source: https://aasnova.org/2017/08/11/have-two-lonely-trans-neptunian-objects-found-each-other/]
Solar System flotsam
Dr. Audrey Thirouin’s main scientific interests are the physical and dynamical properties of the small bodies in the Solar System, such as asteroids, comets, Centaurs, Trojans, and Trans-Neptunian Objects (TNOs). She is particularly interested in the rotational properties of these bodies and what we can learn from them as well as on the rotational properties and the formation of binary and multiple systems in the Trans-Neptunian and asteroid belts. She also works on numerical simulations to explain the formation of families and by extension the genesis of binaries.
Learn more about Dr. Audrey Thirouin