| Discovery[1] | |
|---|---|
| Discovered by | LINEAR |
| Discovery site | Lincoln Lab's ETS |
| Discovery date | 24 August 2003 |
| Designations | |
| Orbital characteristics[2] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 4285 days (11.73 yr) |
| Aphelion | 1.28834 AU (192.733 Gm) |
| Perihelion | 0.882430 AU (132.0096 Gm) |
| 1.08538 AU (162.371 Gm) | |
| Eccentricity | 0.18699 |
| 1.13 yr (413.02 d) | |
Averageorbital speed | 28.34 km/s |
| 264.755° | |
| 0° 52m 17.846s / day | |
| Inclination | 62.1021° |
| 0.997990° | |
| 104.999° | |
| Knownsatellites | S/2021 (143649) 1[3] |
| Earth MOID | 0.00253637 AU (379,436 km) |
| Physical characteristics | |
| Mass | 2.0×1012 kg |
| 2.6446±0.0007 h[3] | |
| 17.4[2] | |
(143649) 2003 QQ47,provisionally designated:2003 QQ47, is a kilometer-sizedasteroid and synchronousbinary system, classified asnear-Earth object andpotentially hazardous asteroid of theApollo group. It became briefly notable upon its discovery in late August 2003, when media outlets played up a very preliminary report that it had a 1 in 250,000 chance ofimpacting intoEarth on 21 March 2014.[4] The discovery of acompanion, approximately 310 meters (1,000 ft) in diameter, was announced in September 2021.
2003 QQ47 was discovered on 24 August 2003.[1] It was added to theSentry Risk Table on 30 August 2003.[4] By 31 August 2003 (with an observation arc of 7 days) the odds of an impact on 21 March 2014 were already reduced to 1 in 1.7 million.[5] The asteroid was removed from the Sentry Risk Table on 14 September 2003, indicating there is no risk of an impact by it in the next 100 years.[6]
2003 QQ47 safely passed within 0.1283 AU (19,190,000 km; 11,930,000 mi) of Earth on 26 March 2014.[2][7] With an observation arc of 10 years and anorbital uncertainty of 0, its orbit and future close approaches are well-determined.[2]
On 3 September 2003 aNASA press release wrote,
Newly discovered asteroid2003 QQ47 has received considerable media attention over the last few days because it had a small chance of colliding with the Earth in the year 2014 and was rated a "1" on theTorino Impact Hazard Scale, which goes from 0 to 10. The odds of collision in 2014, as estimated byJPL's Sentry impact monitoring system, peaked at 1 chance in 250,000, a result which was posted on our Impact Risk Page on Saturday, August 30, 2003. Impact events at the Torino Scale 1 level certainly merit careful monitoring by astronomers, but these events do not warrant public concern. In fact, each year several newly discovered asteroids reach Torino Scale 1 for a brief period after discovery;2003 QQ47 is the fourth such case this year.
On September 2, 2003, new measurements of2003 QQ47's position allowed us to narrow our prediction of its path in 2014, and thus we could rule out any Earth impact possibilities for 2014.[4]
2003 QQ47 has a diameter of approximately 1.24 km, and amass of approximately2.0×1012 kg[citation needed]. If it were to hit the Earth, it would be a major event, with an energy of approximately 350,000megatons ofTNT (1.5 ZJ), enough to cause global damage.
Sara Russell, ameteorite researcher atLondon'sNatural History Museum, told theBBC on 2 September 2003 that she was not worried that2003 QQ47 would be a danger; "The odds are very, very low ... We have to keep some kind of perspective", she said.[8]
As a result of the press coverage of asteroids such as2003 QQ47, astronomers are now planning to re-word the Torino scale, or to phase it out completely in favour of a scale that is less likely to generate false alarms that may reduce public confidence in genuine alerts.
Aminor-planet moon orbiting(143649) 2003 QQ47 was first detected on 29 August 2021, byPetr Pravec,Peter Kušnirák,Kamil Hornoch, and others using photometric data from ESO'sLa Silla Observatory in Chile.[3] The discovery was announced on 17 September 2021. The secondary measures a third the size of its primary (Ds/Dp-ratio of 0.33), resulting in a mean-diameter of approximately 310 meters. It is estimated to be tidally locked, orbiting 1.4 kilometers (4,600 ft) from the primary every 13.065 hours. The primary has arotation period of2.6446±0.0007 hours and a derived diameter of0.94±0.40 kilometers, for a resulting effective diameter (system) of0.995±0.42 kilometers.[3]
