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2021 NASA planetary defense mission

Double Asteroid Redirection Test
Diagram of the DART spacecraft striking Dimorphos
NamesDART
Mission typePlanetary defense test mission
OperatorNASA  / APL
Website
Mission duration
10 months, 1 day
Spacecraft properties
Spacecraft
ManufacturerApplied Physics Laboratory of Johns Hopkins University
Launch mass
  • DART: 610 kg (1,340 lb)[1]
  • LICIACube: 14 kg (31 lb)
Dimensions
  • DART: 1.8 × 1.9 × 2.6 m (5.9 × 6.2 × 8.5 ft)
  • ROSA: 8.5 × 2.4 m (27.9 × 7.9 ft) (each)
Power6.6 kW
Start of mission
Launch date24 November 2021, 06:21:02 (2021-11-24UTC06:21:02Z) UTC[1]
RocketFalcon 9 Block 5 B1063-3
Launch siteVandenberg, SLC4E
ContractorSpaceX
Dimorphos impactor
Impact date26 September 2022, 23:14 UTC[2][3]
Flyby of Didymos system
Spacecraft componentLICIACube (deployed from DART)
Closest approach26 September 2022, ~23:17 UTC
Distance56.7 km (35.2 mi)
Instruments
Didymos Reconnaissance and Asteroid Camera for Optical navigation (DRACO)

Mission logo

The Double Asteroid Redirection Test (DART) was a NASA space mission to test a method of planetary defense against near-Earth objects (NEOs).[4][5] It was designed to assess how much a spacecraft impact can deflect an asteroid by hitting it head-on.[6] The target asteroid, Dimorphos, is a 525 feet (160 m) wide moonlet of the asteroid Didymos; neither asteroid poses an impact threat to Earth, but their joint characteristics made them an ideal target.

Launched on 24 November 2021, the DART spacecraft collided with Dimorphos at 14,000 mph (23,000 km/h) on 26 September 2022 about 6.8 million miles (10.9 million kilometers) from Earth. The collision shortened Dimorphos's orbit around Didymos by 32 minutes, greatly in excess of the pre-defined success threshold of 73 seconds.[7][8][9] Deflection resulted from the ejection of debris which caused a recoil that was substantially larger than the impact itself.[10] The collision also very slightly increased the asteroid pair's orbital speed around the Sun—an effect directly relevant to the goal of planetary protection by changing an object's path through space.

DART was a joint project between NASA and the Johns Hopkins University Applied Physics Laboratory. The project was funded through NASA's Planetary Defense Coordination Office, managed by NASA's Planetary Missions Program Office at the Marshall Space Flight Center, and several NASA laboratories and offices provided technical support. The Italian Space Agency contributed LICIACube, a CubeSat which photographed the impact event, and other international partners, such as the European Space Agency (ESA), and Japan Aerospace Exploration Agency (JAXA), are contributing to related or subsequent projects.[11]

Mission history

[edit]

NASA and the European Space Agency (ESA) started with individual plans for missions to test asteroid deflection strategies, but by 2015, they struck a collaboration called AIDA (Asteroid Impact and Deflection Assessment) involving two separate spacecraft launches that would work in synergy.[12][13][14] Under that proposal, the European Asteroid Impact Mission (AIM), would have launched in December 2020, and DART in July 2021. AIM would have orbited the larger asteroid to study its composition and that of its moon. DART would then kinetically impact the asteroid's moon on 26 September 2022, during a close approach to Earth.[13]

The AIM orbiter was however canceled, then replaced by Hera which plans to start observing the asteroid four years after the DART impact. Live monitoring of the DART impact thus had to be obtained from ground-based telescopes and radar.[15][14]

In June 2017, NASA approved a move from concept development to the preliminary design phase,[16] and in August 2018 the start of the final design and assembly phase of the mission.[17] On 11 April 2019, NASA announced that a SpaceX Falcon 9 would be used to launch DART.[18]

Satellite impact on a small Solar System body had already been implemented once, by NASA's 372-kilogram (820 lb) Deep Impact space probe's impactor spacecraft and for a completely different purpose (analysis of the structure and composition of a comet). On impact, Deep Impact released 19 gigajoules of energy (the equivalent of 4.8 tons of TNT),[19] and excavated a crater up to 150 metres (490 ft) wide.[20]

Description

[edit]

Spacecraft

[edit]

The DART spacecraft was an impactor with a mass of 610 kilograms (1,340 lb)[21] that hosted no scientific payload and had sensors only for navigation. The spacecraft cost US$330 million by the time it collided with Dimorphos in 2022.[22]

Camera

[edit]
DRACO camera

DART's navigation sensors included a Sun sensor, a star tracker called SMART Nav software (Small-body Maneuvering Autonomous Real Time Navigation),[23] and a 20-centimetre (7.9 in) aperture camera called Didymos Reconnaissance and Asteroid Camera for Optical navigation (DRACO). DRACO was based on the Long Range Reconnaissance Imager (LORRI) onboard New Horizons spacecraft, and supported autonomous navigation to impact the asteroid's moon at its center. The optical part of DRACO was a Ritchey-Chrétien telescope with a field of view of 0.29° and a focal length of 2.6208 m (f/12.60). The spatial resolution of the images taken immediately before the impact was around 20 centimeters per pixel. The instrument had a mass of 8.66 kilograms (19.1 lb).[24]

The detector used in the camera was a CMOS image sensor measuring 2,560 × 2,160 pixels. The detector records the wavelength range from 0.4 to 1 micron (visible and near infrared). A commercial off-the-shelf CMOS detector was used instead of a custom charge-coupled device in LORRI. DRACO's detector performance actually met or exceeded that of LORRI because of the improvements in sensor technology in the decade separating the design of LORRI and DRACO.[25] Fed into an onboard computer with software descended from anti-missile technology, the DRACO images helped DART autonomously guide itself to its crash.[26]

Solar arrays

[edit]
The spacecraft's solar arrays used a Roll Out Solar Array (ROSA) design, that was tested on the International Space Station (ISS) in June 2017 as part of Expedition 52.[27]

Using ROSA as the structure, a small portion of the DART solar array was configured to demonstrate Transformational Solar Array technology, which has very-high-efficiency SolAero Inverted Metamorphic (IMM) solar cells and reflective concentrators providing three times more power than other available solar array technology.[28]

Antenna

[edit]

The DART spacecraft was the first spacecraft to use a new type of high-gain communication antenna, a Spiral Radial Line Slot Array (RLSA). The circularly-polarized antenna operated at the (microwave) X-band NASA Deep Space Network (NASA DSN) frequencies of 7.2 and 8.4 GHz, and had a gain of 29.8 dBi on downlink and 23.6 dBi on uplink. The fabricated antenna in a flat and compact shape exceeded the given requirements and was tested through environments resulting in a TRL-6 design.[29]

NASA's Evolutionary Xenon Thruster (NEXT)

Ion thruster

[edit]

DART demonstrated the NEXT gridded ion thruster, a type of solar electric propulsion.[15][30] It was powered by 22-square-metre (240 sq ft) solar arrays to generate the approximately 3.5 kW needed to power the NASA Evolutionary Xenon Thruster–Commercial (NEXT-C) engine.[31] Early tests of the ion thruster revealed a reset mode that induced higher current (100 A) in the spacecraft structure than expected (25 A). It was decided not to use the ion thruster further as the mission could be accomplished without it, using conventional thrusters fueled by the 50 kilograms (110 lb) of hydrazine onboard.[32] However, the ion thrusters remained available if needed to deal with contingencies, and had DART missed its target, the ion system could have returned DART to Dimorphos two years later.[33]

Secondary spacecraft

[edit]
LICIACube CubeSat, a companion satellite of the DART spacecraft

The Italian Space Agency (ASI) contributed a secondary spacecraft called LICIACube (Light Italian CubeSat for Imaging of Asteroids), a small CubeSat that piggybacked with DART and separated on 11 September 2022, 15 days before impact. It acquired images of the impact and ejecta as it drifted past the asteroid.[34][35] LICIACube communicated directly with Earth, sending back images of the ejecta after the Dimorphos flyby.[36][37] LICIACube is equipped with two optical cameras, dubbed LUKE and LEIA.[38]

Effect of the impact on Dimorphos and Didymos

[edit]
Animation of DART around Didymos - Impact on Dimorphos
  DART ·   Didymos ·   Dimorphos

The spacecraft hit Dimorphos in the direction opposite to the asteroid's motion. Following the impact, the instantaneous orbital speed of Dimorphos therefore dropped slightly, which reduced the radius of its orbit around Didymos. The trajectory of Didymos was also modified, but in inverse proportion to the ratio of its mass to the much lower mass of Dimorphos and therefore not much. The actual velocity change and orbital shift depended on the topography and composition of the surface, among other things. The contribution of the recoil momentum from the impact ejecta produces a poorly predictable "momentum enhancement" effect.[39] Before the impact, the momentum transferred by DART to the largest remaining fragment of the asteroid was estimated as up to 3–5 times the incident momentum, depending on how much and how fast material would be ejected from the impact crater. Obtaining accurate measurements of that effect was one of the mission's main goals and will help refine models of future impacts on asteroids.[40]

Scientists later determined that the impact also slightly changed the orbit of the asteroid pair around the Sun--the first time human action measurably had such an effect on a celestial body. The orbital speed increased by about two inches an hour from the pre-impact speed of 76,000 miles per hour (122,000 km/h). Amateur astronomers in several countries contributed data by precisely measuring the pair's occultation of background stars along their orbit after impact. Scientists also used radio telescope data about the pair obtained before and after impact. According to a study author, even such a tiny orbital change might prevent a catastrophic asteroid collision with Earth.[41][42]

The DART impact excavated surface/subsurface materials of Dimorphos, leading to the formation of a crater and/or some magnitude of reshaping (i.e., shape change without significant mass loss). Some of the ejecta may eventually hit Didymos's surface. If the kinetic energy delivered to its surface was high enough, reshaping may have also occurred in Didymos, given its near-rotational-breakup spin rate. Reshaping on either body would have modified their mutual gravitational field, leading to a reshaping-induced orbital period change, in addition to the impact-induced orbital period change. If left unaccounted for, this could later have led to an erroneous interpretation of the effect of the kinetic deflection technique.[43]

Observations of the impact

[edit]
Telescopes observing DART's impact
SOAR telescope shows the vast plume of dust and debris blasted from the surface of the asteroid Dimorphos

DART's companion LICIACube,[44][36] the Hubble Space Telescope, James Webb Space Telescope, and the Earth-based ATLAS observatory all detected the ejecta plume from the DART impact.[45][46] On September 26, SOAR observed the visible impact trail to be over 10,000 kilometres (0.026 LD; 6,200 mi) long.[47] Initial estimates of the change in binary orbit period were expected within a week and with the data released by LICIACube.[48] DART's mission science depends on careful Earth-based monitoring of the orbit of Dimorphos over the subsequent days and months. Dimorphos was too small and too close to Didymos for almost any observer to see directly, but its orbital geometry is such that it transits Didymos once each orbit and then passes behind it half an orbit later. Any observer that can detect the Didymos system therefore sees the system dim and brighten again as the two bodies cross.

The impact was planned for a moment when the distance between Didymos and Earth is at a minimum, permitting many telescopes to make observations from many locations. The asteroid was near opposition and visible high in the night sky well into 2023. The change in Dimorphos's orbit around Didymos was detected by optical telescopes watching mutual eclipses of the two bodies through photometry on the Dimorphos-Didymos pair. In addition to radar observations, they confirmed that the impact shortened Dimorphos's orbital period by 32 minutes.[50] Based on the shortened binary orbital period, the instantaneous reduction in Dimorphos's velocity component along its orbital track was determined, which indicated that substantially more momentum was transferred to Dimorphos from the escaping impact ejecta than from the impact itself. In this way, the DART kinetic impact was highly effective in deflecting Dimorphos.[10]

Follow-up mission

[edit]

In a collaborating project, the European Space Agency has developed Hera, a spacecraft that was launched to Didymos in October 2024[34][51][52] and planned to arrive in 2026[53][54] to do a detailed reconnaissance and assessment.[52] Hera carries two CubeSats, Milani and Juventas.[52]

AIDA mission architecture

[edit]
Host spacecraftSecondary spacecraftRemarks
DARTLICIACube[55]
  • By the Italian Space Agency
  • 6U CubeSat
  • LUKE (LICIACube Unit Key Explorer) Camera and LEIA (LICIACube Explorer Imaging for Asteroid) Camera
Hera Juventas[56][57]
  • By GomSpace and GMV
  • 6U CubeSat orbiter
  • Camera, JuRa monostatic low-frequency radar,[58] accelerometers, and gravimeter[59]
  • Will attempt to land on the asteroid surface57
Milani
  • By Italy/Czech/Finnish consortium
  • 6U CubeSat orbiter
  • VIS/Near-IR spectrometer, volatile analyzer
  • Will characterize Didymos and Dimorphos surface composition and the dust environment around the system
  • Will perform technology demonstration experiments
[edit]

See also

[edit]

Notes

[edit]
  1. The original raw DRACO images from DART were mirror flipped from reality. The images shown in the sequence of operations are uncorrected and show Didymos and Dimorphos as they appear on the DRACO detector.[88]

References

[edit]
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