Potentially hazardous object
A potentially hazardous object (PHO) is a near-Earth asteroid or comet with an orbit such that it has the potential to make close approaches to the Earth and is of a size large enough to cause significant regional damage in the event of impact. A potentially hazardous object with a reasonably well determined orbit can be known not to be a threat to Earth for the next 100 years or more.
As of 1 August 2015[update] NASA had listed a cumulative total of 1,605 discovered potentially hazardous asteroids (PHAs). Among these, there are 154 PHAs believed to be larger than one kilometer in diameter. However a calculated diameter is only a rough estimate, as it is inferred from the object's varying brightness—observed and measured at various times—and the assumed, yet unknown reflectivity of its surface (albedo). Most of the discovered PHAs are Apollo asteroids (1,363) and fewer belong to the group of Aten asteroids (147).
Due to several astronomical surveys, the number of known PHAs has increased tenfold since the end of the 1990s (see bar charts below). These surveys have lead to a total number of 12,933 discovered near-Earth Objects, most of them being asteroids and some 85 near-Earth comets (NECs). The Minor Planet Center's website Unusual Minor Planets also publishes detailed statistics for these objects.
An object is considered a PHO if its minimum orbit intersection distance (MOID) with respect to Earth is less than 0.05 AU (7,500,000 km; 4,600,000 mi)—approximately 19.5 lunar distances—and its diameter is at least 100 to 150 meters (330 to 490 ft)—corresponding to absolute magnitude H < 22. This is big enough to cause regional devastation to human settlements unprecedented in human history in the case of a land impact, or a major tsunami in the case of an ocean impact. Such impact events occur on average around once per 10,000 years. NEOWISE data estimates that there are 4,700 ± 1,500 potentially hazardous asteroids with a diameter greater than 100 meters. As of 2012, an estimated 20 to 30 percent of these objects have been found. Asteroids larger than 35 meters across can pose a threat to a town or city.
The diameter of most small asteroids is not well known and can only be estimated based on their brightness and distance. For this reason NASA and the Jet Propulsion Laboratory use the more practical measure of absolute magnitude (H). Any asteroid with an absolute magnitude of 22.0 or brighter is assumed to be of the required size, although only a coarse estimation of size can be found from the object's magnitude because an assumption must be made for its albedo which is also not usually known for certain. The NASA near-Earth object program uses an assumed albedo of 0.13 for this purpose.
Several astronomical survey projects such as Lincoln Near-Earth Asteroid Research and Catalina Sky Survey continue to search for more PHOs. Each one found is studied by various means, including optical, radar, and infrared to determine its characteristics, such as size, composition, rotation state, and to more accurately determine its orbit. Both professional and amateur astronomers participate in such monitoring.
During an asteroid's close approaches to planets or moons it will be subject to gravitational perturbation, modifying its orbit, and potentially changing a previously non-threatening asteroid into a PHA or vice versa. This is a reflection of the dynamic character of the Solar System.
The largest PHA (based on absolute magnitude H) discovered in a given year:. Historical data of the cumulative number of discovered PHA since 1999 are displayed in the bar charts—one for the total number and the other for objects larger than one kilometer.
The 360-meter PHA (308635) 2005 YU55
- Asteroid-impact avoidance
- Earth-grazing fireball
- Global catastrophic risks
- List of asteroid close approaches to Earth
- "Near-Earth Asteroid Discovery Statistics". Retrieved 2015-08-09.
- "JPL Small-Body Database Search Engine: PHAs and orbital class (APO)". JPL Solar System Dynamics. Retrieved 2014-02-23.
- "JPL Small-Body Database Search Engine: PHAs and orbital class (ATE)". JPL Solar System Dynamics. Retrieved 2014-02-23.
- "Potentially Hazard Asteroids". Retrieved 2011-08-06.
- "Unusual Minor Planets". Minor Planet Center. Retrieved 2012-05-17.
- Agle, DC (19 August 2015). "NASA: There is No Asteroid Threatening Earth". NASA. Retrieved 21 August 2015.
- Chang, Kenneth (20 August 2015). "World Will Not End Next Month, NASA Says". New York Times. Retrieved 20 August 2015.
- Task Force on potentially hazardous Near Earth Objects (September 2000). "Report of the Task Force on potentially hazardous Near Earth Objects" (PDF). Retrieved 2010-06-28.
- "NASA Survey Counts Potentially Hazardous Asteroids". NASA/JPL. May 16, 2012. Retrieved 2012-05-17.
- Will Ferguson (January 22, 2013). "Asteroid Hunter Gives an Update on the Threat of Near-Earth Objects". Scientific American. Retrieved 2013-01-23.
- "Conversion of Absolute Magnitude to Diameter". Minor Planet Center. Retrieved 2009-05-13.
- "JPL Small-Body Database Search Engine: PHAs and H < 18 (mag)". JPL Solar System Dynamics. Retrieved 2012-06-13.
- Sentry Risk Table (current) (NASA NEO Program)
- Very Close Approaches (<0.01 AU) of PHAs to Earth 1800-2200
- TECA Table of Asteroids Next Closest Approaches to the Earth (Sormano Astronomical Observatory)
- MBPL - Minor Body Priority List (PHA Asteroids) (Sormano Astronomical Observatory)
- Responding to the Threat of Potentially-Hazardous Near Earth Objects (PDF)
Minor Planet Center
- List of the Potentially Hazardous Asteroids (PHAs)
- Asteroid Hazards, Part 2: The Challenge of Detection on YouTube (min. 7:14)
- Asteroid Hazards, Part 3: Finding the Path on YouTube (min. 5:38)