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(367789) 2011 AG5, provisional designation 2011 AG5, is a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group.[1] It has a diameter of about 140 meters (460 ft).[4] It was removed from the Sentry Risk Table on 21 December 2012 and as such it now has a rating of 0 on the Torino Scale.[5] As of August 2022, the distance between the orbits of Earth and 2011 AG5 is 0.000025 AU (3,700 km; 0.0097 LD)[1]

Earth Approaches on 3 February 2023 and 4 February 2040[1]
Date JPL Horizons
nominal geocentric
distance (AU)
uncertainty
region
(3-sigma)
2023-Feb-03 08:50 ± 00:020.01215 AU (1.818 million km)[1]±1518 km[6]
2040-Feb-04 08:49 ± 01:230.00713 AU (1.067 million km)[1]±78079 km[7]

(367789) 2011 AG5
Orbital diagram of 2011 AG5 (green) passing the Earth-Moon system in February 2040 (orbital solution from 2011)
Discovery[1][2]
Discovered byMount Lemmon Srvy.
Discovery siteMount Lemon Obs.
Discovery date8 January 2011
Designations
MPC designation
(367789) 2011 AG5
Alternative designations
2011 AG5
Minor planet category
Apollo · NEO · PHA[1][3]
Orbital characteristics[1]
Epoch 2022-Aug-09 (JD 2459800.5)
Uncertainty parameter 1
Observation arc4.84 yr (1,804 days)
Earliest precovery date3 October 2008
Aphelion1.9889 AU
Perihelion0.87209 AU
Semi-major axis
1.4307 AU
Eccentricity0.3905
Orbital period (sidereal)
1.71 yr (625 days)
Mean anomaly
233.21°
Mean motion
0° 34m 33.222s / day
Inclination3.6823°
Longitude of ascending node
135.65°
Time of perihelion
2023-Mar-17
Argument of perihelion
53.589°
Earth MOID0.000025 AU (3,700 km; 0.0097 LD)
Physical characteristics
Dimensions140 m[4]
Mass4×109 kg (assumed)[4]
Absolute magnitude (H)
21.88[3][1]

    Description


    2011 AG5 was discovered on 8 January 2011 by the Mount Lemmon Survey at an apparent magnitude of 19.6 using a 1.52-meter (60 in) reflecting telescope.[3][2] Pan-STARRS precovery images from 8 November 2010 extended the observation arc to 317 days. Observations by the Gemini 8.2-metre (320 in) telescope at Mauna Kea recovered the asteroid on October 20, 21 and 27, 2012,[8] and extended the observation arc to 719 days.[3]

    The October 2012 observations have reduced the orbit uncertainties by more than a factor of 60, meaning that the Earth's position in February 2040 no longer falls within the range of possible future paths for the asteroid.[8] On 4 February 2040 the asteroid will pass no closer than 0.0066 AU (990,000 km; 610,000 mi) (~2.6 LD) from Earth.[1] Until 21 December 2012 it was listed on the Sentry Risk Table with a rating on the Torino Scale of Level 1.[5] A Torino rating of 1 is a routine discovery in which a pass near the Earth is predicted that poses no unusual level of danger.[9] It is estimated that an impact would produce the equivalent of 100 megatons of TNT,[4] roughly twice that of the most powerful nuclear weapon ever detonated (Tsar Bomba). This is powerful enough to damage a region at least a hundred miles wide.


    Older risks


    Virtual clones of the asteroid that fit the mid-2012 uncertainty region in the known trajectory showed four potential impacts between 2040 and 2047.[4] It had a 1 in 500 chance of impacting the Earth on 5 February 2040.[4] In September 2013, there was an opportunity to make additional observations of 2011 AG5 when it came within 0.98 AU (147,000,000 km; 91,000,000 mi) of Earth.[10] The 2013 observations allowed a further refinement to the known trajectory. The asteroid will also pass 0.0121 AU (1,810,000 km; 1,120,000 mi) from the Earth on 3 February 2023.[1][11] The 2023 gravitational keyhole was 227 miles (365 kilometers) wide.[12] With a Palermo Technical Scale of -1.00,[4] the odds of impact by 2011 AG5 were about 10 times less[13] than the background hazard level of Earth impacts which is defined as the average risk posed by objects of the same size or larger over the years until the date of the potential impact.[14]


    References


    1. "JPL Small-Body Database Browser: 367789 (2011 AG5)" (2013-09-11 last obs.). Jet Propulsion Laboratory. Archived from the original on 24 October 2022. Retrieved 24 October 2022.
    2. "MPEC 2011-A31 : 2011 AG5". IAU Minor Planet Center. 9 January 2011. Retrieved 17 October 2011. (K11A05G)
    3. "367789 (2011 AG5)". Minor Planet Center. Retrieved 17 January 2018.
    4. "Earth Impact Risk Summary: 2011 AG5". Wayback Machine: NASA/JPL Near-Earth Object Program Office. Archived from the original on 18 November 2012. Retrieved 12 December 2012.
    5. "Date/Time Removed". NASA/JPL Near-Earth Object Program Office. Archived from the original on 8 January 2013. Retrieved 21 December 2012.
    6. "Horizons Batch for 2023-02-03 Close Approach". JPL Horizons. Archived from the original on 24 October 2022. Retrieved 24 October 2022. RNG_3sigma = uncertainty range in km. (JPL#63/Soln.date: 2021-Jul-11 generates RNG_3sigma = 1518 km)
    7. "Horizons Batch for 2040-02-04 Close Approach". JPL Horizons. Archived from the original on 24 October 2022. Retrieved 24 October 2022. RNG_3sigma = uncertainty range in km. (JPL#63/Soln.date: 2021-Jul-11 generates RNG_3sigma = 78079 km)
    8. ""All Clear" Given on Potential 2040 Impact of Asteroid 2011 AG5". NASA/JPL Near-Earth Object Program Office. 21 December 2012. Archived from the original on 31 December 2012. Retrieved 21 December 2012.
    9. "The Torino Impact Hazard Scale". NASA/JPL Near-Earth Object Program Office. 13 April 2005. Archived from the original on 30 December 2004. Retrieved 5 November 2011.
    10. "Asteroid 2011 AG5 - A Reality Check". NASA/JPL Near-Earth Object Program Office. 28 February 2012. Retrieved 29 February 2012.
    11. "NEODyS-2 Close Approaches for 2011AG5". Near Earth Objects - Dynamic Site. Retrieved 21 September 2013.
    12. "NASA Releases Workshop Data and Findings on Asteroid 2011 AG5". NASA/JPL. 15 June 2012. Retrieved 16 June 2012. (2012-178)
    13. Math: 101.00 = 10
    14. "The Palermo Technical Impact Hazard Scale". NASA/JPL Near-Earth Object Program Office. 31 August 2005. Archived from the original on 21 March 2002. Retrieved 14 October 2011.



    На других языках


    [de] (367789) 2011 AG5

    (367789) 2011 AG5 ist ein erdnaher Asteroid vom Apollo-Typ. Er wurde am 8. Januar 2011 am Mount-Lemmon-Observatorium (Sternwarten-Code G96) der Catalina Sky Survey entdeckt. Seine Umlaufperiode beträgt 1,7 Jahre. Mit einem geschätzten Durchmesser von 140 Metern stellt er eine potentielle Gefahr für die Erde dar und wird auf der Turiner Skala mit der Risikostufe 1 geführt.[1] (367789) 2011 AG5 wird das Erde-Mond-System am 4. Februar 2040 in einer Entfernung von circa 0,007 AE passieren.[2] Dies entspricht einer ungefähren Erdentfernung von einer Million Kilometern.
    - [en] (367789) 2011 AG5

    [es] (367789) 2011 AG5

    El asteroide (367789) 2011 AG5 (también escrito 2011 GA5) es un asteroide cercano a la Tierra y un objeto potencialmente peligroso.[1] Tiene un arco de observación de 256 días, y se encuentra en las listas del sistema de monitoreo Sentry con una clasificación de nivel 1 en la escala de Turín.[3] Una calificación de Torino 1 es un descubrimiento de rutina en el que se prevé que el objeto pase cerca de la Tierra sin presentar un nivel inusual de peligro.[4] El asteroide fue descubierto el 1 de enero de 2011 con un telescopio reflector del Observatorio del Monte Lemmon (Sierra de Santa Catalina, en Arizona).[1] El asteroide tiene un diámetro de más de 140 metros, y esta enlistado por el Centro de Planetas Menores para un potencial acercamiento próximo a la Tierra en el año 2040 con más de 0,001920 UA (287 200 km; 178 500 mi).[5]

    [ru] 2011 AG5

    2011 AG5 — Астероид 367789 2011 AG5 является потенциально опасным. Размер астероида может достигать 250 метров. Открыт 3 октября 2008 года.



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