 moment—including the moment of impact.
Most of our past observations of Didymos come from 2003 when the binary made a close approach to Earth and was bright enough to be observed by a large number of ground-based telescopes. Since then, it has only gotten bright enough to be observed by the largest telescopes. The latest observing window just ended in early April 2019. Since late January, Didymos was bright enough to be observed from a handful of large telescopes (V21.0). The team knew this was a great opportunity to get more observations!
We started planning our observing effort in the summer of 2018 at the Didymos Observers Workshop. Our international team gathered to discuss what data we had from past observing windows, the quality of data needed to reach our goals, and which telescopes could be used to achieve these goals. From that discussion we generated a list of telescopes that our group would propose to use in the 2019 observing window. These proposals were due in the fall and we spent the next couple of months hoping that we had made our case clear to the telescope allocation committees.
We were fortunate enough to get 11.5 nights on six large telescopes ranging from the 4.3-meter Discovery Channel Telescope in Arizona to the 10.4-meter Gran Telescopio Canarias on the Canary Islands (Spain). For the last three months, many people have worked hard to plan the observing, take the observations, calculate the lightcurves, and include the newest lightcurves into models of the Didymos system. And we've been trying to work fast! When the impact happens in 2022, the telescope data will need to be studied quickly so we can share the results with other team members.
As with most observing programs, not all of our nights were successful—we had high winds, high humidity and scheduling issues throughout. Overall though, we had several nights of great data and I'm looking forward to seeing the final results of our effort.
I already know that we will still have so much to learn. Didymos will be bright enough to observe again in mid-2020 for approximately eight months. In fact, it'll be even brighter than it was earlier this year and our team is looking forward to repeating the process again.
Beyond DART, our observations will help us better understand near-Earth asteroid binary systems. About 15% of near-Earth asteroids are thought to be binary systems, so they're a small, but notable amount of the population. The shape of Didymos A and the orbit of Didymoon have already contributed to our understanding of the formation of these systems and our future observations will help us understand their current evolution.
It's been a while since I first imagined sending a spacecraft to Didymos. A decade ago, I was in a mission design summer school at NASA Ames Research Center as a graduate student with a dozen other students with a wide range of scientific interests. Of that small group, four of us are now actively involved in DART and it has been really exciting to see how far we've all come. I know we're all excited for DART's impact in 2022!