 2004 XP14 imaged by theGoldstone Solar System Radar in 2006 | |
| Discovery | |
|---|---|
| Discovered by | LINEAR |
| Discovery date | 10 December 2004 |
| Designations | |
| NEO · Apollo · PHA | |
| Orbital characteristics[1] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 1007 days (2.76 yr) |
| Aphelion | 1.21822 AU (182.243 Gm) |
| Perihelion | 0.884900 AU (132.3792 Gm) |
| 1.05156 AU (157.311 Gm) | |
| Eccentricity | 0.158488 |
| 1.08yr (393.87d) | |
| 10.1555° | |
| 0° 54m 50.45s /day | |
| Inclination | 32.9505° |
| 281.045° | |
| 273.695° | |
| Earth MOID | 0.00316799 AU (473,925 km) |
| Physical characteristics | |
| 130–260 m[2] 300–800 m[3] | |
| 100 h (4.2 d)[1] | |
| 19.4[1] | |
(612901) 2004 XP14 is a sub-kilometerasteroid, classified as anear-Earth object andpotentially hazardous asteroid of theApollo group. It was first observed by theLINEAR project on 10 December 2004.
Although initially there were concerns that it might possibly impactEarth later in the 21st century and thus merit special monitoring, further analysis of its orbit has since ruled out any such collision, at least in the foreseeable future.
The size of2004 XP14 is not precisely known. Based on optical measurements, the object is between 300 and 800 meters in diameter.[1]Radar observations place a lower bound of about 260 meters (850 ft).[2]
2004 XP14's closest pass by Earth was above the west coast of North America at 04:25 UTC on 3 July 2006.[1]
The asteroid's distance from Earth's center of mass at that moment was 0.0028906 AU (432,430 km; 268,700 mi),[1] or just 1.1 times theMoon's average distance from Earth. It was observed immediately after this close approach byradar from three locations, fromGoldstone in theMojave Desert in the US, fromSicily, and fromYevpatoria RT-70 radio telescope,Ukraine, as well as optically from other observatories[4] and amateurs.
It was removed from theSentry Risk Table on 17 March 2005.[5]
| Asteroid | Date | Nominal approach distance (LD) | Min. distance (LD) | Max. distance (LD) | Absolute magnitude (H) | Size (meters) |
|---|---|---|---|---|---|---|
| (152680) 1998 KJ9 | 1914-12-31 | 0.606 | 0.604 | 0.608 | 19.4 | 279–900 |
| (458732) 2011 MD5 | 1918-09-17 | 0.911 | 0.909 | 0.913 | 17.9 | 556–1795 |
| (163132) 2002 CU11 | 1925-08-30 | 0.903 | 0.901 | 0.905 | 18.5 | 443–477 |
| 69230 Hermes | 1937-10-30 | 1.926 | 1.926 | 1.927 | 17.5 | 668–2158 |
| 69230 Hermes | 1942-04-26 | 1.651 | 1.651 | 1.651 | 17.5 | 668–2158 |
| (27002) 1998 DV9 | 1975-01-31 | 1.762 | 1.761 | 1.762 | 18.1 | 507–1637 |
| 2002 NY40 | 2002-08-18 | 1.371 | 1.371 | 1.371 | 19.0 | 335–1082 |
| 2004 XP14 | 2006-07-03 | 1.125 | 1.125 | 1.125 | 19.3 | 292–942 |
| 2015 TB145 | 2015-10-31 | 1.266 | 1.266 | 1.266 | 20.0 | 211–682 |
| (137108) 1999 AN10 | 2027-08-07 | 1.014 | 1.010 | 1.019 | 17.9 | 556–1793 |
| (153814) 2001 WN5 | 2028-06-26 | 0.647 | 0.647 | 0.647 | 18.2 | 921–943 |
| 99942 Apophis | 2029-04-13 | 0.0981 | 0.0963 | 0.1000 | 19.7 | 310–340 |
| 2017 MB1 | 2072-07-26 | 1.216 | 1.215 | 2.759 | 18.8 | 367–1186 |
| 2011 SM68 | 2072-10-17 | 1.875 | 1.865 | 1.886 | 19.6 | 254–820 |
| (163132) 2002 CU11 | 2080-08-31 | 1.655 | 1.654 | 1.656 | 18.5 | 443–477 |
| (416801) 1998 MZ | 2116-11-26 | 1.068 | 1.068 | 1.069 | 19.2 | 305–986 |
| (153201) 2000 WO107 | 2140-12-01 | 0.634 | 0.631 | 0.637 | 19.3 | 427–593 |
| (276033) 2002 AJ129 | 2172-02-08 | 1.783 | 1.775 | 1.792 | 18.7 | 385–1242 |
| (290772) 2005 VC | 2198-05-05 | 1.951 | 1.791 | 2.134 | 17.6 | 638–2061 |
