Where’s Lucy Going? Studying Asteroid Mission Targets

Title: Light Curves of Lucy Targets: Leucus and Polymele

Authors: Marc W. Buie, Amanda M. Zangari, Simone Marchi, Harold F. Levison, Stefano Mottola

First Author’s Institution: Southwest Research Institute

Status: Published in ApJ, June 2018 (closed access)

Asteroids, meteoroids, meteors, meteorites. Usually when we talk about these small chunks of debris and rock in the solar system, it’s about another possible apocalypse scenario. Studies of rocky objects that may pass near Earth’s orbit (Near Earth Objects, or NEOs) are of obvious importance for the safety of humanity, but they are only one minor subset of the small bodies in our solar system. Most of the asteroids in our neighborhood live in the Asteroid Belt, a region between the orbits of Mars and Jupiter, and are referred to as “main belt asteroids”. There are also large populations trailing Jupiter in its orbit (the Trojan asteroids) and floating out in the outer solar system near Neptune (the Centaur asteroids).

            But apart from the potential threat caused by NEOs, why study these plentiful, seemingly uninteresting hunks of rock and metal that we will likely never encounter on Earth? It turns out that they actually serve as an important window into the formation of the solar system, providing us with information on how the planets formed and what our early solar system was made of. Since we have the chance to get up-close and personal with the planets and asteroids nearest to us with rovers and other probes, scientists use this information to infer how other planetary systems form as well. In recent history, we’ve visited most of the major planets with satellites, such as Voyager or Cassini, or rovers, such as Curiosity on Mars; however, the smaller debris is still largely unexplored. The New Horizons flyby in 2015 provided a glimpse into icy debris in the outer solar system when it imaged Pluto in detail for the first time, and both NASA’s OSIRIS-REx and JAXA’s Hayabusa missions are working on returning samples from Near-Earth asteroids.

            A new asteroid mission has begun preparation as well, targeting multiple asteroids in the further-out Trojan group near Jupiter. The Lucy Discovery mission plans to visit multiple Trojans (actually, the largest number of independently orbiting objects ever visited by a single probe), including Leucus and Polymele, whose flybys are scheduled for September 2027 and April 2028 respectively. Until that date, though, astronomers are busy preparing for the mission and trying to gather all the data on these objects that we can from Earth. The authors specifically investigate Leucus and Polymele, using their light curves to tease out information about their color, composition, orbit, and reflectivity.

            A light curve traces the variation in the light we receive from an object over time, and for asteroids, we’re mostly seeing light reflected from the Sun. One of the key parameters, then, is how reflective the asteroid’s surface is – its albedo. Tracing the variations in intensity and finding periodic patterns can also determine the rotation period of an asteroid; imperfections in the surface lead to bumps and wiggles in the light curve, and by tracking how long it takes to see the same imperfection again, we find how long the asteroid takes to rotate around its own axis. By collecting light in different wavelengths, astronomers can also derive colors, comparisons of how much light we get at one wavelength versus another.

            For Leucus and Polymele, this research group used telescopes in the Las Cumbres Global Telescope Network (LCOGT), specifically two telescopes at Cerro Tololo in Chile and one at McDonald Observatory in the United States. These images were taken in the red part of the spectrum of visible light, since asteroids tend to be brighter at longer wavelengths. After taking multiple data images over time, the results of the brightness of the asteroid vs. time are plotted into a light curve, as shown in Figure 1.

Figure 1 – A Light Curve for Leucus, clearly showing its rotational variability. (Figure 6 in the paper)

            Through their observations of Leucus, the team determined that it has a very long rotation period, and may actually be a binary system. Future observations from the ground will be needed to determine if it is or not. From its colors, Leucus is also determined to be a D-type asteroid, one of the less common types. Asteroids are grouped into a few main categories based on their composition (e.g. carbonaceous (C-type), silicaceous (S-type), metallic (M-type); D-type, or “primitive” asteroids are very dark (even darker than coal!), and may be interesting to how life began on Earth because they are thought to carry organic, carbon-rich material. Unfortunately, this paper reports that Polymele is still not well-understood, likely because it is so small and might be nearly spherical; that is, there isn’t much variation in its light curve, and it’s also extremely dark, though not as dark as Leucus.

Figure 1 – A Light Curve for Polymele. (Figure 10 in the paper)

            Although these may seem like small steps at first, determining characteristics of one or two rocks in the vast solar system, they are actually stepping stones (literally!) to understanding the population of asteroids that surrounds us. Asteroids may be what brought life to Earth, and they are intact remnants of the story of planet formation. The key to a successful space mission is minimizing risk, and a large component of that is knowing what you’re getting into when you’re millions of miles away in space; studying these asteroids will prevent the spacecraft from encountering physical hazards (like collisions), and will inform what data we need to take in-situ to better understand them. By studying the future targets of the Lucy mission now, the lander, and the humans running the mission, will be prepared for its eventual encounter with them.

About Briley Lewis

Briley Lewis is a PhD Candidate and NSF Fellow at the University of California, Los Angeles studying Astronomy & Astrophysics. Her research interests are primarily in planetary systems – both exoplanets and objects in our own solar system, how they form, and how we can create instruments to learn more about them. She has previously pursued her research at the American Museum of Natural History in NYC, and also at Space Telescope Science Institute in Baltimore, MD. Outside of research, she is passionate about teaching and public outreach, and spends her free time bringing together her love of science with her loves of crafting and writing, and playing with her rescue dog Rocky.

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