NASA’s new planet finder is in space. Now what?

Most everyone reading this story will probably know that a SpaceX Falcon 9 rocket launched on Wednesday carrying a NASA spacecraft into orbit—the Transiting Exoplanet Survey Satellite—that will further the space agency’s mission of searching for exoplanets.

Less well known is the TESS spacecraft’s clever orbit, which will enable an on-a-budget but robust science mission of searching for planets transiting in front of nearby stars. This “lunar resonant” orbit, which has never been used by a spacecraft, will allow TESS to both observe nearby stars and transmit data back to Earth with a minimal energy expenditure. (The useful lifetime of a spacecraft is often determined by its amount of onboard propellant).

Lunar resonant orbit

Science missions often need continuous and unobstructed views of their targets, and TESS is no different, as it will monitor about 200,000 relatively nearby stars for minuscule changes in their brightness. NASA’s previous planet-hunter that searched for similar transits, the Kepler mission, observed its targets from an Earth-trailing, heliocentric orbit about 10 million km from our planet. Such an orbit has high costs in terms of energy needed to reach it, station keeping, and data limitations.

The orbit sequence for TESS: first, a parking orbit (green), followed by a phasing orbit (yellow) with a lunar gravity assist which puts TESS into its final orbit (red), which is in a 2:1 resonance with the Moon (orbit in white).

Science in 60 days

After this week’s launch, it will take a couple of weeks for TESS to reach this stable orbit, as the spacecraft performs half a dozen thruster burns and utilizes a gravity assist from the Moon to reach its desired orbit. After that, it will undergo about two months of checkouts before beginning science operations.

At a cost of $200 million, the TESS spacecraft is about one-third the cost of the Kepler spacecraft, which had a main mirror with a diameter of 0.95 meter. The TESS apertures are considerably smaller: 10cm for four identical cameras. Its advantage is that, whereas Kepler observed a small area of the sky, TESS will look at much more, about 85 percent in total.