New tracking data confirms that NASA's OSIRIS-REx spacecraft aced its first Deep Space Maneuver (DSM-1) on Dec. 28, 2016. The engine burn sets up the spacecraft for an Earth gravity assist this fall as it continues its two-year journey to the asteroid Bennu.

The large maneuver was the first using OSIRIS-REx's main engines and resulted in a 964 miles per hour (431 meters per second) change in the vehicle's velocity utilizing 780 pounds (354 kilograms) of fuel.

Tracking data from the Deep Space Network (DSN) confirmed the successful maneuver, and subsequent downlink of high-rate telemetry from the spacecraft shows that all subsystems performed as expected.

"DSM-1 was our first major trajectory change and first use of the main engines, so it's good to have that under our belts and be on a safe trajectory to Bennu," said Arlin Bartels, deputy project manager at NASA's Goddard Space Flight Center in Greenbelt, Maryland.

DSM-1 represents the first major, post-launch milestone for OSIRIS-REx. The significant change in trajectory from DSM-1 was necessary to put OSIRIS-REx on course for an encounter with Earth in September of this year.

A smaller trajectory correction maneuver will be executed on Wednesday, Jan. 18 to refine the course for the Earth flyby, during which Earth's gravity will bend the OSIRIS-REx trajectory and slinging it toward a rendezvous with the asteroid Bennu in the fall of 2018.

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NASA's first mission to return a sample of an asteroid to Earth will be multitasking during its two-year outbound cruise to the asteroid Bennu. On Feb. 9-20, the OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security- Regolith Explorer) spacecraft will activate its onboard camera suite and commence a search for elusive "Trojan" asteroids.

Trojans are asteroids that are constant companions to planets in our solar system as they orbit the sun, remaining near a stable point 60 degrees in front of or behind the planet. Because they constantly lead or follow in the same orbit, they will never collide with their companion planet.

There are six planets in our solar system with known Trojan asteroids-Jupiter, Neptune, Mars, Venus, Uranus and, yes, even Earth. The Earth Trojan is elusive; to date, scientists have only discovered one Earth trojan asteroid - 2010 TK7 - found by NASA's NEOWISE project in 2010. Yet there are more than 6,000 known Trojans that are co-orbiting the sun with the gas giant Jupiter.

Scientists predict that there should be more Trojans sharing Earth's orbit, but these asteroids are difficult to detect from Earth because they appear close to the sun from Earth's point of view. In mid-February 2017, however, the OSIRIS-REx spacecraft will be positioned in an ideal spot to undertake a survey.

Over 12 days, the OSIRIS-REx Earth-Trojan asteroid search will employ the spacecraft's MapCam imager to methodically scan the space where Earth Trojans are expected to exist. Many of these observations will closely resemble MapCam's planned activities during its upcoming search for satellites of asteroid Bennu, so the Trojan asteroid search serves as an early rehearsal for the mission's primary science operations.

"The Earth-Trojan asteroid search provides a substantial advantage to the OSIRIS-REx mission," said OSIRIS-REx Principal Investigator Dante Lauretta of the University of Arizona, Tucson. "Not only do we have the opportunity to discover new members of an asteroid class, but more importantly, we are practicing critical mission operations in advance of our arrival at Bennu, which ultimately reduces mission risk."

The OSIRIS-REx spacecraft is currently on a seven-year journey to rendezvous with, study, and bring a sample of Bennu to Earth. This sample of a primitive asteroid will help scientists understand the formation of our solar system more than 4.5 billion years ago.