Since its launch in March 2009, the Kepler Space Telescope has provided us with an incredible amount of data about exoplanets within our galaxy, proving these worlds are more varied and numerous than we could ever have imagined. Before its launch we simply didn’t know how common planets such as ours were, but today we know the Milky Way contains billions of them. Some of these worlds are so hot they have seas of molten rock, others experience two sunsets a day as they orbit a pair of stars. Perhaps most importantly, thousands of the planets found by Kepler are much like our own: potentially playing host to life as we know it.

Kepler lived a fruitful life by any metric, but it hasn’t been an easy one. Too far into deep space for us to repair it as we did Hubble, hardware failures aboard the observatory nearly brought the program to a halt in 2013. When NASA announced the spacecraft was beyond hope of repair, most assumed the mission would end. Even by that point, Kepler was an unqualified success and had provided us with enough data to keep astronomers busy for years. But an ingenious fix was devised, allowing it to continue collecting data even in its reduced capacity.

Leaning into the solar wind, Kepler was able to use the pressure of sunlight striking its solar panels to steady itself. Kepler’s “eyesight” was never quite the same after the failure of its reaction wheels, and it consumed more propellant than originally intended to maintain this careful balancing act, but the science continued. The mission that had already answered many of our questions about our place in the galaxy would push ahead in spite of a failure which should have left it dead in space.

As Kepler rapidly burned through its supply of propellant, it became clear the mission was on borrowed time. It was a necessary evil, as the alternative was leaving the craft tumbling through space, but mission planners understood that the fix they implemented had put an expiration date on Kepler. Revised calculations could provide an estimate as to when the vehicle would finally run its tanks dry and lose attitude control, but not a definitive date.

For the last several months NASA has known the day was approaching, but they decided to keep collecting data until the vehicle’s thrusters sputtered and failed. So today’s announcement that Kepler has at long last lost the ability to orient itself came as no surprise. Kepler has observed its last alien sunset, but the search for planets, and indeed life, in our corner of the galaxy doesn’t end today.

Kepler Phones Home

NASA has been especially careful these last few months to regularly download collected data from the spacecraft; knowing that each download could be their last. When the propellant ran out and Kepler was no longer able to orient itself towards its targets, it would also no longer be able to reliably point its high-gain antenna at Earth. When properly oriented, Kepler was capable of transmitting data back to Earth at roughly 4.3 Mbps (unusually high bandwidth for a deep space craft), but on the low end data rates could drop to a single byte per second. Leaving Kepler adrift in space with a trove of valuable data locked in its onboard storage would have been a particularly undignified end to the mission, so NASA made sure no data was left behind.

The data collected up to this last observation session (referred to as Campaign 19) will keep scientists busy for years. NASA expects the amount of data they’ve pulled down from Kepler to date will yield at least 1,000 scientific papers in coming years, and estimate it will be at least another decade before all of the data has been analyzed. They note that just this summer, a paper was published that used data from 2016’s Campaign 10 observations to identify an additional 44 planets.

A Bright Future

Not only is there a decade of Kepler data to sort though still, but NASA’s next generation planet hunting telescope, the Transiting Exoplanet Survey Satellite (TESS) is already in space. Launched aboard a SpaceX Falcon 9 on April 18, 2018, TESS began its primary science mission a few months later and has already started identifying candidate exoplanets. Utilizing the same transit observation method as Kepler, where the light from target stars is carefully monitored to detect the telltale dimming when a planet obscures it, TESS will be able to monitor a section of the sky roughly 400 times greater than that of its predecessor.

Understandably, expectations are very high. Given the wealth of data Kepler collected watching its relatively small slice of the galaxy, the sky is quite literally the limit for TESS. It won’t be working alone either, the planets discovered by TESS will be considered prime targets for the James Webb Space Telescope when it comes online. This combination of discovery and analysis by the two complementary spacecraft promise to improve our ability to directly image exoplanets, which to date has been very limited.

Between the data directly collected during its lifetime, and the successor missions which make use of techniques pioneered by Kepler, we’re looking at 20 to 30 years of discoveries. The conclusion of Kepler’s mission is therefore not the end of an era, but the beginning of a new one; which promises to redefine our knowledge of the galaxy and our place in it.