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65803 Didymos

From Wikipedia, the free encyclopedia
Near-Earth asteroid
For other uses, seeDidymos.

65803 Didymos
Didymos (bottom left) andDimorphos (top right) photographed by theDART space probe
Discovery[1]
Discovered bySpacewatch
Discovery siteKitt Peak National Observatory
Discovery date11 April 1996
Designations
(65803) Didymos
Pronunciation/ˈdɪdɪmɒs/[2]
Named after
Greek word for "Twin"[3]
1996 GT
NEO · PHA
Apollo (2022)[1][a]
Orbital characteristics[1]
Epoch 21 January 2022 (JD 2459600.5)
Uncertainty parameter 0
Observation arc24.82 years (9,066 days)
Aphelion2.2753AU
Perihelion1.0131 AU
1.6442 AU
Eccentricity0.38385
2.11yr (770 days)
232.01
0° 28m 2.28s / day
Inclination3.4079°
73.196°
319.32°
Knownsatellites1 (Dimorphos)
Earth MOID0.0403 AU (15.7 LD)
Mars MOID0.02 AU (7.8 LD)[4]
Physical characteristics[5]
Dimensions851 × 849 × 620 m
15 × 15 × 15 m)
765±15 m[b]
Mass(5.4±0.4)×1011 kg (system)[6]
≈5.2×1011 kg (primary)[7]
2.40±0.30 g/cm3[5]
2.2600±0.0001[6]
2.2593±0.0002 h[8]
174°±20°[c]
310°±20°
−84°±20°
0.15±0.04
S[6][10] · SMASS =Xk[1] · X[11]
18.0[1] · 18.16[11][8][12]
18.16±0.03[13]

65803 Didymos (provisional designation1996 GT) is a sub-kilometerasteroid andbinary system that is classified as apotentially hazardous asteroid andnear-Earth object of theApollo group.[a] The asteroid was discovered in 1996 by theSpacewatch survey atKitt Peak, and its small 160-meterminor-planet moon, namedDimorphos, was discovered in 2003. Due to its binary nature, the asteroid was then namedDidymos, theGreek word for 'twin'.

Didymos's moon,Dimorphos, was the target of theDART mission to test the viability ofasteroid impact avoidance by collision with a spacecraft, while the impact was witnessed byLICIACube, a flybyCubeSat component of the mission.

Discovery

[edit]
Radar images of Didymos and its satelliteDimorphos, taken by theArecibo Observatory in 2003

Didymos was discovered on 11 April 1996 by theUniversity of ArizonaSteward Observatory's, andLunar and Planetary Laboratory's,Spacewatch survey using its 0.9-meter telescope atKitt Peak National Observatory in Arizona, United States. The binary nature of the asteroid was discovered by others; suspicions of binarity first arose inGoldstone delay-Doppler echoes, and these were confirmed with an opticallightcurve analysis, along withArecibo radar imaging on 23 November 2003.[4]

Orbital characteristics

[edit]

Didymos orbits the Sun at a distance of 1.0–2.3AU once every 770 days (2 years and 1 month). Its orbit has aneccentricity of 0.38 and aninclination of 3° with respect to theecliptic. The minimum distance between the orbit of Earth and the orbit of Didymos is currently 0.04 AU (6.0 million km),[1] but will change as the asteroid isperturbed. In November 2003 it passed 7.18 million km from Earth; it will not come that near again until November 2123, with a distance of 5.86 million km. Didymos also occasionally passes very close to Mars: it will fly by Mars at a distance of 4.68 million km in July 2144.[1] The Earth approach of October 2184, at a distance of 8.6 million km, is listed with an uncertainty region of roughly ±105 km.[14]

Didymos spends one third of its time orbiting far enough from the Sun to cross the inner parts of themain asteroid belt, where collisions with other asteroids are more probable. This means that about every 73–84 thousand years, an object impacts Didymos with the energy of theDART mission satellite. Over its median NEA lifetime of 8 to 10 million years, Didymos probably has been hit several tens of times.[15]

Physical characteristics

[edit]
Dust ejecta and tail of Didymos imaged in color by theSouthern Astrophysical Research Telescope two days after DART's impact
Double tail of Didymos imaged by theHubble Space Telescope 12 days after DART's impact

In theSMASS classification, Didymos was classified as an Xk-type asteroid, which transitions from theX-type to the rareK-type asteroids.[1] Subsequent visible and near-infrared spectroscopy showed it to be silicate in nature, which also qualifies it as a stonyS-type asteroid.[16] Itrotates rapidly, with a period of 2.26 hours and a low brightness variation of 0.08magnitude (U=3/3), which indicates that the body has a nearly spheroidal shape.[11][8][17] Radar observations confirmed this spheroidal shape, showing it to beoblate due to its rapid rotation.[6]

Satellite

[edit]
Main article:Dimorphos

Didymos is abinary asteroid with a satellite in its orbit. Theminor-planet moon, namedDimorphos,[18] moves in a mostly circularretrograde orbit[19] with anorbital period of 11.9 hours.[11][d] It measures approximately 160 meters (520 ft) in diameter compared to 780 meters (2,560 ft) for its primary (amean diameter-ratio of 0.22).[20] It was previously known by itsprovisional designationS/2003 (65803) 1 and had been informally called "Didymoon" or "Didymos B".[21][18]

Naming

[edit]

Thisminor planet was named "Didymos", Greek for "twin", due to its binary nature.[3] The name was suggested by the discoverer,University of ArizonaLunar and Planetary Laboratory astronomerJoseph L. "Joe" Montani, who made the naming proposal to theInternational Astronomical Union after the binary nature of the object was detected. The approved naming citation was published on 13 July 2004 (M.P.C. 52326).[22]

The proper name for the satelliteDidymos B comes from the word "Dimorphos", Greek for "having two forms".[23] The meaning of the name represents how the form of Dimorphos's orbit will change after the collision with NASA's Double Asteroid Redirection Test (DART) spacecraft,[18] though in fact the change will be only a very slight change in its orbital parameters. Appropriately, Dimorphos serves dual roles as both a test target and as a part of a blueprint for a modality for future planetary protection.[18] The name of the moon was suggested by planetary scientistKleomenis Tsiganis at theAristotle University of Thessaloniki, Greece.[24]

Two boulders (saxa) have been given names of traditional drums.[25]

Named features
NamePronunciationFeatureNamed afterDate approved[25]
Carillon SaxumUS:/ˈkærəlɒn/
UK:/kəˈrɪljən/
bouldercarillon14 Nov 2023
Gong Saxum/ˈɡɒŋ/bouldergong14 Nov 2023

Exploration

[edit]
Telescope image of Didymos before DART's impact
Artist's impression of theDART spacecraft
Timelapse of the Didymos system's expanding dust plume from the DART impact, as seen by theSouth African Astronomical Observatory's 1-meter Lesedi telescope
Animation of DART's trajectory
  DART ·   65803 Didymos ·   Earth ·   Sun ·   2001 CB21 ·   3361 Orpheus
Animation of DART around Didymos - Impact on Dimorphos
  DART ·   Didymos ·   Dimorphos

In the early 2010s, Didymos's moon, Dimorphos was to be the principal target of proposed robotic mission by theESA andNASA, called theAsteroid Impact & Deflection Assessment (AIDA) mission. The ESA dropped out, and the mission did not proceed.[26][27]

NASA redefined mission requirements and decided to proceed with a 2020s mission to visit Didymos with an impactor, which had been considered as a part of the earlier AIDA mission, named theDouble Asteroid Redirection Test or DART. The NASA mission was intended to test whether a spacecraft impact could successfully deflect an asteroid on a collision course with Earth. The DART spacecraft was launched on 24 November 2021, and impacted Dimorphos on September 26, 2022.[28][29][30] It was accompanied by theItalian Space Agency's (ASI) six-unitLICIACube flybyCubesat that was released 15 days before impact to observe the asteroid and DART's impact.[31]

DART was the first spacecraft to intentionally target and successfully visit an asteroid known to have aminor-planet moon (The binary asteroid2000 DP107 was targeted by thePROCYON mission before it failed,243 Ida was visited by theGalileo spacecraft but its moon was unknown until then,Pluto was considered a planet until a few months after the launch ofNew Horizons, and3548 Eurybates's and15094 Polymele's moons were not discovered until months before and afterLucy's launch, respectively). Didymos is the most easily reachable asteroid of its size from Earth, requiring adelta-v of only5.1 km/s for a spacecraft to rendezvous, compared to6.0 km/s to reach theMoon.[32]

After two weeks of analysis, NASA announced that the collision shortened Dimorphos's orbital period around Didymos by 32 minutes,[33] far more than the minimum requirement of 73 seconds and the success benchmark of 10 minutes. The measurement has an uncertainty of ±2 minutes.[34]

Dart Impact seen by LICIACube

Another mission to Didymos was approved in November 2019 and launched in October 2024, with the arrival at Didymos being expected in 2026.[35] ESA'sHera mission is planning to survey the dynamical effects of the DART impact and measure the characteristics of the crater made by DART.[36]

See also

[edit]

Notes

[edit]
  1. ^abIt is anApollo asteroid becauseperihelion (q) is less than 1.017 AU (Earth aphelion), not greater.
  2. ^Volume-equivalent spherical diameter is calculated from an ellipsoid's volume given Didymos's dimensions of851 × 849 × 620 m,[5]: 28–29  and then solving for radius withr=3V4π3{\displaystyle r={\sqrt[{3}]{3V \over 4\pi }}}.
  3. ^Naidu et al. (2020) give the Didymos's north pole direction in terms ofecliptic coordinates, whereλ is ecliptic longitude andβ is ecliptic latitude.[6]: 12 β is the angular offset from the ecliptic plane whereas inclinationi with respect to the ecliptic is the angular offset from the ecliptic north pole atβ = +90°;i with respect to the ecliptic would be thecomplement ofβ.[9] Therefore, givenβ = –84°,i = 90° – (–84°) = 174° from the ecliptic.
  4. ^Lightcurve plots of 65803 Didymos, Palmer Divide Observatory,B. D. Warner

References

[edit]
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  2. ^"didymous".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abSchmadel, Lutz D. (2006). "(65803) Didymos [1.64, 0.38, 3.4]".Dictionary of Minor Planet Names – (65803) Didymos, Addendum to Fifth Edition: 2003–2005.Springer Berlin Heidelberg. p. 225.doi:10.1007/978-3-540-34361-5_2677.ISBN 978-3-540-34361-5.
  4. ^ab"65803 Didymos (1996 GT)".Minor Planet Center.Archived from the original on 12 November 2020. Retrieved12 March 2017.
  5. ^abcCheng, Andrew F.; et al. (2023)."Momentum transfer from the DART mission kinetic impact on asteroid Dimorphos".Nature.616 (7957):457–460.arXiv:2303.03464.Bibcode:2023Natur.616..457C.doi:10.1038/s41586-023-05878-z.PMID 36858075. (This work is licensed under a CC BY 4.0 License)
  6. ^abcdeNaidu, S. P.; Benner, L. A. M.; Brozovic, M.; Nolan, M. C.; Ostro, S. J.; Margot, J. L.; et al. (September 2020)."Radar observations and a physical model of binary near-Earth asteroid 65803 Didymos, target of the DART mission"(PDF).Icarus.348 113777.Bibcode:2020Icar..34813777N.doi:10.1016/j.icarus.2020.113777.S2CID 219091858. 134777.
  7. ^Nakano, Ryota; Hirabayashi, Masatoshi; Brozovic, M.; Nolan, M. C.; Ostro, S. J.; Margot, J. L.; et al. (July 2022)."NASA's Double Asteroid Redirection Test (DART): Mutual Orbital Period Change Due to Reshaping in the Near-Earth Binary Asteroid System (65803) Didymos".The Planetary Science Journal.3 (7): 16.Bibcode:2022PSJ.....3..148N.doi:10.3847/PSJ/ac7566.S2CID 250327233. 148.
  8. ^abcPravec, P.; Scheirich, P.; Kusnirák, P.; Sarounová, L.; Mottola, S.; Hahn, G.; et al. (March 2006)."Photometric survey of binary near-Earth asteroids".Icarus.181 (1):63–93.Bibcode:2006Icar..181...63P.doi:10.1016/j.icarus.2005.10.014.Archived from the original on 3 October 2022. Retrieved12 March 2017.
  9. ^"Coordinate transformations".Astronomy and Astrophysics. European Southern Observatory. January 1998.Archived from the original on 17 June 2021. Retrieved17 June 2022.
  10. ^Scheirich, P.; Pravec, P. (July 2022)."Preimpact Mutual Orbit of the DART Target Binary Asteroid (65803) Didymos Derived from Observations of Mutual Events in 2003–2021".The Planetary Science Journal.3 (7): 12.Bibcode:2022PSJ.....3..163S.doi:10.3847/PSJ/ac7233.S2CID 250650906. 163.
  11. ^abcd"LCDB Data for (65803) Didymos". Asteroid Lightcurve Database (LCDB).Archived from the original on 1 July 2020. Retrieved12 March 2017.
  12. ^Kitazato, K.; Abe, M.; Mito, H.; Tarusawa, K.; Soyano, T.; Nishihara, S.; et al. (March 2004)."Photometric Behaviour Dependent on Solar Phase Angle and Physical Characteristics of Binary Near-Earth-Asteroid (65803) 1996 GT".35th Lunar and Planetary Science Conference. p. 1623.Bibcode:2004LPI....35.1623K.Archived from the original on 3 October 2022. Retrieved12 March 2017.
  13. ^Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved12 March 2017.
  14. ^"Horizons Batch for 2184-Oct-14 Close Approach".JPL Horizons.Archived from the original on 20 December 2024. Retrieved14 October 2022. RNG_3sigma = uncertainty range in km. (JPL#194/Soln.date: 2022-Oct-13 generates RNG_3sigma = 1343 km)
  15. ^Campo Bagatin, Adriano; Dell'Oro, Aldo; Parro, Laura M.; Benavidez, Paula G.; Jacobson, Seth; Lucchetti, Alice; Marzari, Francesco; Michel, Patrick; Pajola, Maurizio; Vincent, Jean-Baptiste (3 May 2024)."Recent collisional history of (65803) Didymos".Nature Communications.15 (1): 3714.Bibcode:2024NatCo..15.3714C.doi:10.1038/s41467-024-48094-7.ISSN 2041-1723.PMC 11068898.PMID 38702317.
  16. ^de León, J.; Licandro, J.; Serra-Ricart, M.; Pinilla-Alonso, N.; Campins, H. (28 July 2010)."Observations, compositional, and physical characterization of near-Earth and Mars-crosser asteroids from a spectroscopic survey".Astronomy and Astrophysics.517: A23.Bibcode:2010A&A...517A..23D.doi:10.1051/0004-6361/200913852.
  17. ^Pravec, P.; Benner, L. A. M.; Nolan, M. C.; Kusnirak, P.; Pray, D.; Giorgini, J. D.; et al. (November 2003)."(65803) 1996 GT".IAU Circular (8244): 2.Bibcode:2003IAUC.8244....2P.Archived from the original on 3 October 2022. Retrieved12 March 2017.
  18. ^abcdTalbert, Tricia (23 June 2020)."NASA's First Planetary Defense Mission Target Gets a New Name". NASA.Archived from the original on 10 February 2021. Retrieved23 June 2020.Public Domain This article incorporates text from this source, which is in thepublic domain.
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  20. ^Johnston, Robert (20 September 2014)."(65803) Didymos". johnstonsarchive.net.Archived from the original on 23 October 2020. Retrieved28 June 2017.
  21. ^"Telescopes focus on target of ESA's asteroid missionArchived 18 August 2015 at theWayback Machine" at phys.org (30 June 2015)
  22. ^"MPC/MPO/MPS Archive".Minor Planet Center.Archived from the original on 7 January 2022. Retrieved12 March 2017.
  23. ^"MPEC 2020-M83 : (65803) Didymos I = Dimorphos".Minor Planet Center. International Astronomical Union. 23 June 2020.Archived from the original on 8 October 2021. Retrieved23 June 2020.
  24. ^"IAU Approves Name of Target of First NASA and ESA Planetary Defence Missions". International Astronomical Union. 23 June 2020.Archived from the original on 26 September 2021. Retrieved23 June 2020.
  25. ^ab"Nomenclature Search Results".planetarynames.wr.usgs.gov.
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  27. ^"Asteroid Impact & Deflection Assessment". ESA.Archived from the original on 19 March 2018. Retrieved28 June 2017.
  28. ^Warren, Haygen (26 September 2022)."Brace for impact: DART successfully slams into asteroid".NASASpaceFlight.com.Archived from the original on 27 September 2022. Retrieved27 September 2022.
  29. ^"DART Sets Sights on Asteroid Target".NASA. 7 September 2022.Archived from the original on 21 September 2022. Retrieved20 September 2022.
  30. ^Potter, Sean (23 November 2021)."NASA, SpaceX Launch DART: First Test Mission to Defend Planet Earth".NASA.Archived from the original on 24 November 2021. Retrieved25 November 2021.
  31. ^Greshko, Michael (23 November 2021)."This NASA spacecraft will smash into an asteroid—to practice saving Earth".National Geographic. Archived fromthe original on 23 November 2021. Retrieved25 November 2021.
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  33. ^"NASA says DART's asteroid impact was a huge success".The Planetary Society. Retrieved11 October 2022.
  34. ^"NASA Confirms DART Mission Impact Changed Asteroid's Motion in Space".NASA. 11 October 2022. Retrieved11 October 2022.
  35. ^"Planetary defence mission Hera heading for deflected asteroid".www.esa.int. Retrieved7 October 2024.
  36. ^Numerical modelling of the DART impact and the importance of the Hera mission. Sabina D. Raducan, Thomas M. Davison, Gareth S. Collins. PDC 2019. Washington, D.C., USA.

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