| Minorplanet: | yes |
| 2019 OK | |
| Background: |
|
| Discovery Ref: |   |
| Discovery Site: | SONEAR Obs. |
| Discovered: | 24 July 2019 |
| Mpc Name: | 2019 OK |
| Alt Names: | NEOCP S511618 |
| Orbit Ref: |   |
| Epoch: | 27 April 2019 (JD 2458600.5) |
| Uncertainty: | 1 |
| Observation Arc: | 2.42 years |
| Earliest Precovery Date: | 2017-02-21 (Pan-STARRS) |
| Perihelion: | 0.4635 AU |
| Semimajor: | 1.9475 AU |
| Eccentricity: | 0.7620 |
| Period: | 2.72 yr (993 d) |
| Mean Motion: | / day |
| Inclination: | 1.4006° |
| Asc Node: | 302.27° |
| Arg Peri: | 104.24° |
| Moid: | 0.00036AU (0.14 LD) |
| Mean Diameter: | NaNabbr=onNaNabbr=on |
| Abs Magnitude: | 23.3 |
2019 OK is a near-Earth asteroid noted for its sudden, surprise discovery on the day before it flew by at approximately 70000km (40,000miles) in 2019.[1] The object's size is estimated at 187to across, the closest asteroid of such size discovered in 2019.[2] It is uncommon for asteroids of this moderately large size to pass within 100000km (100,000miles) of Earth.
The first detection made public occurred on 24 July 2019, when it was 0.01AU from Earth and had an apparent magnitude of 14.7. The full moon on 16 July 2019 slowed down the asteroid discovery rate during mid-July. The asteroid was detected by Cristóvão Jacques, Eduardo Pimentel and João Ribeiro at the private SONEAR Observatory in Oliveira, Minas Gerais when it was very close to opposition (opposite the Sun in the sky) with a solar elongation of 170 degrees. About 10 hours later it was independently detected by ASAS-SN project in images from two of its telescopes, which allowed a preliminary determination of its orbit. It was subsequently listed on the Minor Planet Center's Near-Earth Object Confirmation Page (NEOCP) as S511618. The listing was confirmed and publicly announced as 2019 OK with three hours remaining before the 25 July 2019 closest approach.
Various circumstances prevented an earlier discovery, despite the efforts to continuously hunt for such objects. The last previous appearance was not lost in the glare of the Sun, but was not favorable to survey instruments located in the Northern Hemisphere, due to its celestial direction in the Southern constellation Capricornus and close to the bright moon. The Pan-STARRS1 telescope did record an image of 2019 OK on 28 June 2019 when it was 0.39AU from Earth and had an apparent magnitude of 22.9. Automatic analysis missed detecting the object in the Pan-STARRS image because the object was too faint. The Pan-STARRS1 telescope again saw the object on 7 July 2019 when the object was brighter with magnitude 21.2. However, it was at that time moving directly towards the observer and its apparent motion across the sky was extremely slow, with a rate of 0.01 degrees/day, and it was not recognized as a moving object.
The asteroid is a member of the Flora family, a populous asteroid family and the largest family of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 0.5–3.4 AU once every 2 years and 9 months (993 days; semi-major axis of 1.95 AU). Its orbit has an eccentricity of 0.76 and an inclination of 1° with respect to the ecliptic. After evaluating its orbit, the asteroid was identified as the most probable parent body of the particles responsible for the meteor shower designated, 17 Capricornids (SCP #1042).
On 25 July 2019 at 01:22 UTC it had its closest approach to Earth, when it passed about 0.00047697AU—less than one-fifth of the distance to the Moon. Its speed was nearly 88500km (55,000miles) per hour.[3] [4]
On 28 July 2116 the asteroid will pass about 0.03AU from Earth.| 2019 OK | 2019-07-25 | 71 | 23.3 | 75 | |
| 2019 OD | 2019-07-24 | 357 | 23.5 | 68 | |
| 2018-05-15 | 202 | 23.6 | 65 | ||
| 2018-04-15 | 192 | 23.8 | 60 | ||
| 2018-01-02 | 296 | 22.5 | 110 | ||
| 2013-02-15 | 34 | 24.0 | 54 | ||
| 2011-12-03 | 347 | 23.2 | 79 | ||
| 2011-11-08 | 324 | 21.9 | 140 |
Asteroids in the 20m (70feet) Chelyabinsk meteor size range to 50m (160feet) Tunguska size range (absolute magnitude H ~26–24) approach closer than the Moon about once per month. Asteroids with an absolute magnitude of 26–24 will vary in size from 17to depends on the objects albedo (how reflective it is).[5]
If 2019 OK is around 100m (300feet) in diameter, an Earth impact could have released as much power as the 50 megatons generated by the Tsar Bomba hydrogen bomb.[6] If 2019 OK is around the middle of the size estimates, it could instead have released the equivalent explosive energy of about 10 megatons of TNT similar to the 1908 Tunguska event that flattened 2,000 km2 (770 square miles) of forest land.[4] If 2019 OK is on the smaller size it still could have released over 30 times the energy of the atomic blast by Little Boy at Hiroshima.[7]