Space Matter: Where We Came From

Space Matter(s) is a weekly column that delves into space science and the mechanics of spaceflight. From the latest discoveries in the universe around us to the fits and starts of rocket test flights, you’ll find analysis, discussion, and an eternal optimism about space and launching ourselves into the cosmos.
Sometimes it’s easy to forget that NASA is a large organization, with goals beyond human spaceflight. There are smaller and less-splashy programs within NASA doing incredibly important work in furthering our understanding of the world and universe around us. One such program is NASA’s Discovery, which began in 1992, that accepts submissions from teams of scientists and engineers to figure out where it should send robotic spacecraft. It was a real and pivotal shift in how NASA approached missions, and it’s had incredible effects.
These missions don’t replace the larger, more headline-grabbing (and more expensive) robotic spacecraft missions NASA does; they’re complementary. The idea is that the Discovery missions are lower cost, quicker to launch, and often utilize breakthroughs in technology to achieve their goals. It’s a ingenious program that has had great results—it gets the scientific, engineering, and educational public more invested in NASA, helps NASA do more with the resources it has, and furthers science.
Some Discovery programs you’ve likely heard of? Mars Pathfinder, the rover launched in 1996 and was celebrated by The Martian, as Mark Watney used the lander to communicate with Earth. Kepler, a personal favorite, the planet-hunting spacecraft that has discovered exoplanets large and small, and is still chugging along, three years after its primary mission concluded. These may not be the fanciest of missions, but they have helped us make advances in science and occasionally, even captured the imagination and attention of the public at large, no small feat.
Last week, NASA announced the selection of two new Discovery missions, out of an incredible roster of candidates. Let’s take a more in-depth look at what was chosen, why, and what they could tell us about the universe we live in.
The first mission, Lucy, is headed for the asteroid belt. The current schedule is to launch in October of 2021, and to arrive in 2025. The mission will last until 2033, during which Lucy will explore six Jupiter Trojan asteroids. The Trojan asteroids are a cluster of asteroids, each with unique features, that orbit two Lagrangian points. A Lagrange point is an area between two larger bodies (in this case, Jupiter and the Sun) where a third body (in this case, the Trojan asteroids) can maintain a stable position due to the forces of gravity—think of it as a parking spot in space. There are five total Lagrangian points within the solar system.
Three Lagrangian points—L1, L2, and L3—are unstable. This means that any shift in direction would result in objects at that Lagrangian point falling towards one of the two bodies affecting it. For example, the James Webb telescope (Hubble’s replacement) is scheduled to be launched to the L2 Lagrangian point in 2018. If it were nudged out of place, it would fall either towards the sun or Earth, without being able to regain its former stability. Lagrangian points L4 and L5, however, are stable (and therefore, attractive possible locations for future space stations/space colonies)—a nudge towards the sun, say, would be offset by a pull from Jupiter, and it would be able to rebalance. That’s where Lucy is heading.