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OSIRIS-REx

OSIRIS-REx was a NASA asteroid-study and sample-return mission that visited and collected samples from 101955 Bennu, a carbonaceous near-Earth asteroid. The material, returned in September 2023, is expected to enable scientists to learn more about the formation and evolution of the Solar System, its initial stages of planet formation, and the source of organic compounds that led to the formation of life on Earth. Following the completion of the primary OSIRIS-REx mission, the spacecraft, renamed as OSIRIS-APEX, began a follow-up mission to asteroid 99942 Apophis.

Mission
Overall management, engineering, and navigation for the OSIRIS missions are provided by NASA Goddard Space Flight Center, while the University of Arizona Lunar and Planetary Laboratory provides principal science operations. Lockheed Martin Space Systems built the spacecraft and provides mission operations. After traveling for approximately two years, the spacecraft rendezvoused with asteroid 101955 Bennu in December 2018, and began 505 days of surface mapping at a distance of approximately . Then a close approach (without landing) was carried out to allow extension of a robotic arm to gather the sample. Following the successful collection of material (), the sample was returned to Earth in a capsule similar to that which returned the samples of Comet 81P/Wild on the space probe Stardust. The return trip to Earth was shorter than the outbound trip. The capsule landed by parachute at the Utah Test and Training Range on 24 September 2023 and was transported to the Johnson Space Center for processing in a dedicated research facility. OSIRIS-REx separated from the launch vehicle 55 minutes after ignition. Cruise phase OSIRIS-REx entered the cruise phase shortly after separation from the launch vehicle, following successful solar panel deployment, propulsion system initiation, and establishment of a communication link with Earth. On 28 December 2016, the spacecraft successfully performed its first deep space maneuver to change its velocity by using of fuel. An additional, smaller firing of its thrusters on 18 January 2017 further refined its course for an Earth gravity assist on 22 September 2017. as it closely resembled the operation required as the spacecraft approached Bennu, searching for natural satellites and other potential hazards. On 12 February 2017, while from Jupiter, the PolyCam instrument aboard OSIRIS-REx successfully imaged the giant planet and three of its moons, Callisto, Io, and Ganymede. OSIRIS-REx flew by Earth on 22 September 2017. Arrival and survey On 3 December 2018, NASA confirmed that OSIRIS-REx had matched the speed and orbit of Bennu at a distance of about , effectively reaching the asteroid. OSIRIS-REx performed closer passes of the Bennu surface, initially at about through December to further refine the shape and orbit of Bennu. Preliminary spectroscopic surveys of the asteroid's surface by the OSIRIS-REx spacecraft detected the presence of hydrated minerals in the form of clay. While researchers suspect that Bennu was too small to host water, the hydroxyl groups may have come from water present in its parent body before Bennu split off. OSIRIS-REx entered orbit around Bennu on 31 December 2018 at about to start its extensive remote mapping and sensing campaign for the selection of a sample site. This is the closest distance that any spacecraft has orbited a celestial object, closer than the Rosetta orbit of comet 67P/Churyumov–Gerasimenko at . At this altitude, it took the spacecraft 62 hours to orbit Bennu. At the end of its detailed survey, the spacecraft entered a closer orbit with a radius of . Sample acquisition Procedure Rehearsals were performed before sampling, during which the solar arrays were raised into a Y-shaped configuration to minimize the chance of dust accumulation during contact and provide more ground clearance in case the spacecraft tipped over (up to 45°) during contact. Upon surface contact by the TAGSAM instrument, a burst of nitrogen gas was released to blow regolith particles smaller than into the sampler head at the end of the robotic arm. A five-second timer limited the collection time to mitigate the chance of a collision, and the probe then executed a back-away maneuver to depart safely. In addition to the bulk sampling mechanism, contact pads on the end of the sampling head made of tiny stainless steel loops (Velcro) passively collected dust grains smaller than . Operations NASA selected the final four candidate sample sites in August 2019, named Nightingale, Kingfisher, Osprey, and Sandpiper. On 12 December 2019, they announced that Nightingale had been selected as the primary sample site and Osprey was selected as the backup site. Both were within craters, with Nightingale near Bennu's north pole while Osprey was near the equator. NASA planned to perform the first sampling in late August 2020; NASA's originally planned Touch-and-Go (TAG) sample collection was scheduled for 25 August 2020, but was rescheduled for 20 October 2020, at 22:13 UTC. On 15 April 2020, the first sample collection rehearsal was successfully performed at the Nightingale sample site. The exercise took OSIRIS-REx as close as from the surface before performing a back-away burn. A second rehearsal was successfully completed on 11 August 2020, bringing OSIRIS-REx down to from the surface. This was the final rehearsal before the sample collection scheduled for 20 October 2020, at 22:13 UTC. At 22:13 UTC, on October 20, 2020, OSIRIS-REx successfully touched down on Bennu at a distance of from Earth. NASA confirmed via images taken during sampling that the sampler had made contact. The spacecraft touched down within of the target location. A sample of the asteroid which was estimated to weigh at least was collected by OSIRIS-REx following the touch down. When the head was seated into the Sample-Return Capsule's capture ring on 28 October 2020, the spacecraft performed a "backout check", which commanded the TAGSAM arm to back out of the capsule. This maneuver is designed to tug on the collector head and ensure that the latches – which keep the collector head in place – are well secured. Following the test, the mission team received telemetry confirming that the head was properly secured in the Sample-Return Capsule. Thereafter, on 28 October 2020, two mechanical parts on the TAGSAM arm were disconnected – these are the tube that carried the nitrogen gas to the TAGSAM head during sample collection and the TAGSAM arm itself. Over the next several hours, the mission team commanded the spacecraft to cut the tube that stirred up the sample through the TAGSAM head during sample collection, and separate the collector head from the TAGSAM arm. Once the team confirmed these activities were done, it commanded the spacecraft on 28 October 2020, to close and seal the Sample-Return Capsule, the final step of the sample stowage process of Bennu's samples. To seal the SRC, the spacecraft closed the lid and then secured two internal latches. On inspecting images, it was observed that a few particles had escaped from the collector head during the stowage procedure, but it was confirmed that no particles would hinder the stowage process, since the team was confident that a plentiful amount of material remained inside of the head, more than the needed, that is, . The sample of Bennu was safely stored and ready for its journey to Earth. With the collector head secure inside the SRC, pieces of the sample would no longer be lost. Sample return On 7 April 2021, OSIRIS-REx completed its final flyover of Bennu and began drifting away from the asteroid. On 10 May 2021, the spacecraft departed the vicinity of Bennu and began its two-year journey to Earth with the asteroid sample. On 24 September 2023, at 4:42 a.m. MDT, at a distance of from Earth, it ejected the sample return capsule, which re-entered the atmosphere at . Due to a mistake in wiring, the drogue parachute did not deploy as planned at 100,000 feet (30,400 meters). However, the main parachute was released when the spacecraft reached about 9,000 feet (2,700 meters), and it survived deployment despite higher than anticipated speeds. The main spacecraft maneuvered to a trajectory away from Earth for its extended mission to Apophis in 2029 called OSIRIS-APEX. At 10:15 a.m. MDT, the capsule was taken from the landing site by helicopter. The sample will be analyzed at NASA's Astromaterials Research and Exploration Science Directorate (ARES) and at Japan's Extraterrestrial Sample Curation Center. Asteroid sample material requests will be considered and distributed to organizations worldwide by ARES. On 11 October 2023, the recovered capsule was opened to reveal a "first look" at the asteroid sample contents. Further looks were reported on 13 December 2023 and revealed organic molecules and unknown materials that require study to determine their composition. Some damaged fasteners prevented immediate opening, but, after three months, on 13 January 2024, NASA reported fully opening the recovered container. In total, of asteroidal material was recovered from the sample container. The samples became available to the world’s scientists for research by request on 1 April 2024. On 15 May 2024, an overview of preliminary analytical studies on the returned samples was reported. In January 2025, NASA revealed that while the samples did not show evidence of life, their contents suggest that the conditions necessary for the emergence of life were likely widespread in the early solar system. The amount of ammonia, a volatile substance, in the samples indicates that Bennu emerged from the colder, outer regions of space. ==Extended mission OSIRIS-APEX==
Extended mission OSIRIS-APEX
On 25 April 2022, NASA confirmed that the mission would be extended. After dropping off its sample to Earth on 24 September 2023, the mission became OSIRIS-APEX (Apophis Explorer). OSIRIS-APEX will orbit Apophis for around 18 months in a regime similar to that at Bennu. The spacecraft will perform a maneuver, similar to sample collection at Bennu, by using its thrusters to disturb Apophis's surface, in order to expose and spectrally study the subsurface and the material beneath it. The mission, initially proposed to be shut down with the FY2026 budget, was saved after legislators included continued funding for the project in the bill. == Name ==
Name
OSIRIS-REx and OSIRIS-APEX are acronyms, and each letter or combination of letters relates to part of the respective projects: • O – Origins • SI – Spectral Interpretation • RI – Resource Identification • S – Security • REx – Regolith Explorer • APEX – Apophis Explorer Each of these words was chosen to represent an aspect of this mission. The mission name itself was a reference to the god Osiris. Dante Lauretta, deputy PI of the mission, was called "a mythology buff" by the mission PI Michael Drake: "he was doodling on a pad and trying to capture the principal themes of what we are trying to do with this mission—study life origins, identify resources, planetary security in the form of asteroid deflection—and he realized he got the name of Osiris out of that, an ancient god of Egypt who may have been one of the first pharaohs." Similar to how Osiris in mythology taught agriculture to humanity which brought civilization and life to Egypt, OSIRIS-REx aims to return samples from an asteroid that may contain organics that led to the origin of life on Earth. Rex is the Latin word for king which is a reference to Osiris being a mythical king of Egypt. Asteroid Bennu is named after the mythological bird from ancient Egyptian mythology that was associated with the Sun and the creation of the cosmos, while the asteroid for the second mission is named after the ancient Egyptian god Apophis, who was associated with chaos and destruction. Both asteroids Bennu and Apophis are named after figures in Egyptian mythology just like OSIRIS-REx. == Science objectives ==
Science objectives
The science objectives of the mission are: • Return and analyze a sample of pristine carbonaceous asteroid regolith in an amount sufficient to study the nature, history, and distribution of its constituent minerals and organic compounds • Map the global properties, chemistry, and mineralogy of a primitive carbonaceous asteroid to characterize its geologic and dynamic history and provide context for the returned samples • Document the texture, morphology, geochemistry, and spectral properties of the regolith at the sampling site in situ at scales down to millimeters • Measure the Yarkovsky effect (a thermal force on the object) on a potentially hazardous asteroid and constrain the asteroid properties that contribute to this effect • Characterize the integrated global properties of a primitive carbonaceous asteroid to allow for direct comparison with ground-based telescopic data of the entire asteroid population Telescopic observations have helped define the orbit of 101955 Bennu, a near-Earth object (NEO) with a mean diameter in the range of . It completes an orbit of the Sun every 436.604 days (1.2 years). This orbit takes it close to the Earth every six years. Although the orbit is reasonably well known, scientists continue to refine it. It is critical to know the orbit of Bennu because recent calculations produced a cumulative probability of 1 in 1410 (or 0.071%) of impact with Earth from 2169 to 2199. One of the mission objectives is to refine understanding of non-gravitational effects (such as the Yarkovsky effect) on this orbit, and the implications of those effects for Bennu's collision probability. Knowing Bennu's physical properties will be critical for future scientists to understand when developing an asteroid impact avoidance mission. == Specifications ==
Specifications
• Dimensions: Length , width , height • The sample-return capsule reentered the Earth's atmosphere with a parachute assisted landing. The capsule with encased samples was retrieved from Earth's surface and is being studied, as was done with the Stardust mission. == Instruments ==
Instruments
In addition to its telecommunication equipment, the spacecraft carries a suite of instruments to image and analyze the asteroid on many wavelengths, OCAMS The OSIRIS-REx Camera Suite (OCAMS) consists of the PolyCam, the MapCam, and the SamCam. Together, they acquire information on asteroid Bennu by providing global mapping, sample site reconnaissance and characterization, high-resolution imaging, and records of the sample acquisition. • PolyCam, an telescope, acquired visible-light images with increasingly higher resolution on approach the asteroid and high-resolution surface images from orbit • MapCam searches for satellites and outgassing plumes. It maps the asteroid in four blue, green, red and near infrared channels, and informs the model of Bennu's shape and provides high resolution imaging of the potential sample sites • SamCam continuously documents the sample acquisitions OVIRS The OSIRIS-REx Visible and IR Spectrometer (OVIRS) is a spectrometer which maps minerals and organic substances on the asteroid's surface. This data was used in concert with OTES spectra to guide sample-site selection. The spectral ranges and resolving powers are sufficient to provide surface maps of carbonates, silicates, sulfates, oxides, adsorbed water and a wide range of organic compounds. OTES The OSIRIS-REx Thermal Emission Spectrometer (OTES) provides thermal emission spectral maps and local spectral information of candidate sample sites in the thermal infrared channel covering 4–50 μm, again to map mineral and organic substances. REXIS is a coded aperture soft X-ray (0.3–7.5 keV) telescope that images X-ray fluorescence line emission produced by the absorption of solar X-rays and the solar wind by elements in the regolith of Bennu leading to local X-ray emissions. Images were formed with 21 arcminute resolution (4.3 m spatial resolution at a distance of 700 m). Imaging was achieved by correlating the detected X-ray image with a 64×64 element random mask (1.536 mm pixels). REXIS stored data for each X-ray event to maximize data storage usage and minimize the risk. The pixels were addressed in 64×64 bins and the 0.3–7.5 keV range was covered by five broad bands and 11 narrow line bands. A 24-second resolution time tag was interleaved with the event data to account for Bennu rotation. Images were reconstructed on the ground after downlink of the event list. Images were formed simultaneously in 16 energy bands centered on the dominant lines of abundant surface elements from O-K (0.5 keV) to Fe-Kß (7 keV) as well the representative continuum. During orbital phase 5B, a 21-day orbit 700 m from the surface of Bennu, a total of at least 133 events/asteroid pixel/energy band were expected under 2 keV; enough to obtain significant constraints on element abundances at scales larger than 10 m. On 11 November 2019, while observing the asteroid with REXIS, university students and researchers involved in the mission unexpectedly discovered an X-ray burst from a black hole named MAXI J0637-430 located 30,000 light-years away. OLA The OSIRIS-REx Laser Altimeter (OLA) is a scanning and lidar instrument that will provide high resolution topographical information throughout the mission. OLA was delivered for integration with the spacecraft on 17 November 2015. The lead instrument scientist of OLA is Michael Daly from York University. TAGSAM The sample-return system, called Touch-And-Go Sample Acquisition Mechanism (TAGSAM), consists of a sampler head with an articulated arm. • Contact within of selected location • OCAMS documents sampling at 1 Hz • Collect samples in less than five seconds, direct nitrogen (N2) annular jet fluidizes regolith, surface-contact pad captures surface sample • Verify bulk sample collection via spacecraft inertia change; surface sample by imaging sampler head • Sampler head stored in sample-return capsule and returned to Earth == Cooperation with JAXA ==
Cooperation with JAXA
Hayabusa2 is a similar mission from JAXA to collect samples from near-Earth asteroid 162173 Ryugu. It arrived at the asteroid in June 2018, left in November 2019 after two successful sample collections, and returned to Earth in December 2020. The recovery capsule of Hayabusa2 re-entered Earth atmosphere and landed in Australia, as planned, on 5 December 2020. The sample contents were to be extensively analyzed, including water content, to provide clues on the initial formation of the asteroid. The main module of Hayabusa2 is performing a swing-by procedure to "push" it onward to its next destination, asteroid 1998KY26, by 2031. Because the two missions were similar and had overlapping timelines (OSIRIS-REx was still in the return phase), NASA and JAXA signed an agreement to collaborate on sample exchange and research. The two teams visited each other, with representatives from JAXA visiting the OSIRIS-REx Science Operations Center at the University of Arizona, and members of the OSIRIS-REx team traveling to Japan to meet with the Hayabusa2 team. The teams are sharing software, data, and techniques for analysis, and will eventually exchange portions of the samples that are returned to Earth. == OSIRIS-REx II ==
OSIRIS-REx II
OSIRIS-REx II was a 2012 mission concept to replicate the original spacecraft for a double mission, with the second vehicle collecting samples from the two moons of Mars, Phobos and Deimos. It was stated that this mission would be both the quickest and least expensive way to get samples from the moons. Mars I and II are now the aims of another mission, led by JAXA, called MMX, to be launched in 2026. == Gallery ==
Gallery
File:Tour of Asteroid Bennu.webm|Narrated tour of Bennu's most prominent surface features, as seen by OSIRIS-REx File:Asteroid Bennu's Surprising Surface Revealed by OSIRIS-REx (long form).webm|Effects of OSIRIS-REx sampling attempt on Bennu OSIRIS-REx_First_Image_of_Asteroid_Bennu.gif|First images of asteroid Bennu (August 2018) OSIRIX-REx views Asteroid Bennu.jpg|Asteroid Bennu from away (29 October 2018) NASA-EarthMoonLowerLeft-BennuAsteroidUpperRight-20190108.jpg|Earth-Moon (lower left) and asteroid Bennu (upper right) (December 2018) OSIRIS-REx SRC and Bennu.png|The Sample Return Capsule (SRC) with asteroid Bennu in the background (December 2019) OSIRIS-REx Sampling Before and After (Dated Frames).gif|The "Nightingale" sample site pictured before and after the sampling maneuver File:Maps14227-fig-0004-m.jpg|The opened return capsule File:OSIRIS-REx sample at Space Center Houston.jpg|Sample being displayed at Space Center Houston == See also ==
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