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Yesterday’s trajectory-correction maneuver changed the spacecraft’s velocity about a ½ mph (less than 1 kph) relative to Earth. Without this tiny but critical shift, the spacecraft and its asteroid cargo would have flown past Earth.
But now, the spacecraft is set up to release the capsule to enter the atmosphere just off the coast of California at 8:42 a.m. MDT / 10:42 a.m. EDT.
Traveling at a precise speed and angle, it will land approximately 13 minutes after release in a 36-mile by 8.5-mile (58-kilometer by 14-kilometer) predetermined area on the Department of Defense’s Utah Test and Training Range southwest of Salt Lake City.
Meanwhile, about 20 minutes after releasing the sample capsule, the spacecraft will fire its engines to divert past Earth and onto its next mission to asteroid Apophis: OSIRIS-APEX (OSIRIS-Apophis Explorer).
OSIRIS-REx may fire its thrusters again on Sept. 17 if engineers determine that one final adjustment to its trajectory is necessary before it releases its capsule a week later.
The spacecraft is currently 4 million miles, or 7 million kilometers, away, traveling at about 14,000 mph (about 23,000 kph) toward Earth.
blogs.nasa.gov...
originally posted by: gortex
...
But now, the spacecraft is set up to release the capsule to enter the atmosphere just off the coast of California at 8:42 a.m. MDT / 10:42 a.m. EDT.
Traveling at a precise speed and angle, it will land approximately 13 minutes after release in a 36-mile by 8.5-mile (58-kilometer by 14-kilometer) predetermined area on the Department of Defense’s Utah Test and Training Range southwest of Salt Lake City.
originally posted by: Brotherman
a reply to: gortex
Hopefully it ushers in a new era, the space zombie apocalypse.
Was that second mission directive planed from the start?
“The investigation is not without substantial technical risk,” Lori Glaze, director of NASA’s planetary science division, wrote in an April 25 memo approving the extension. The trajectory OSIRIS-APEX will take will bring it within half an astronomical unit of the sun, much closer than originally designed when the spacecraft traveled to Bennu, requiring what she called “significant engineering work” to ensue spacecraft systems can survive several such close approaches before arriving at Apophis.
www.eoportal.org...-apex-origins-spectral-interpretation-resource-identification-and-security-apophis- explorer
How close will apophis pass and will their thruster burn change it's trajectory?
Why bring samples home when the ship can analyze on-board?
Will it stay with apophis or return home?
Though calcite is the most common carbonate mineral that we identify on Bennu, at least one-quarter of the carbonate detections are more Mg-rich compositions based on the wavelength of their 3.4-μm features (Fig. 3), including likely dolomite, breunnerite, and magnesite.
Carbonaceous asteroids formed early in Solar System history and experienced varying degrees of aqueous (water-rock) and thermal alteration. Most models of the evolution of these asteroids suggest that aqueous alteration was driven by hydrothermal convection. However, it is debated whether this alteration occurred in a chemically closed or open system. The bulk chemical compositions of the carbonaceous chondrite meteorites imply that the system was closed. Models predict that large-scale fluid flow in an open system took place on at least some asteroids. In this scenario, fluids would have flowed through fractures from the interior, and minerals would have precipitated into these fractures, forming veins.