1972 Great Daylight Fireball Explained

Place:Northern America

The Great Daylight Fireball (also known as the Grand Teton Meteor) was an Earth-grazing fireball that passed within 57km (35miles) of Earth's surface at 20:29 UTC on August 10, 1972. It entered Earth's atmosphere at a speed of 15km/s in daylight over Utah, United States (14:30 local time) and passed northwards leaving the atmosphere over Alberta, Canada. It was seen by many people and recorded on film and by space-borne sensors.[1] An eyewitness to the event, located in Missoula, Montana, saw the object pass directly overhead and heard a double sonic boom. The smoke trail lingered in the atmosphere for several minutes.

The atmospheric pass modified the object's mass and orbit around the Sun. A 1994 study found that it is probably still in an Earth-crossing orbit and predicted that it would pass close to Earth again in August 1997.[2] However, the object has not been observed again and so its post-encounter orbit remains unknown.[3]

Description

Analysis of its appearance and trajectory showed the object was about 3to in diameter, depending on whether it was a comet made of ice or a stony and therefore denser asteroid. Other sources identified it as an Apollo asteroid in an Earth-crossing orbit that would make a subsequent close approach to Earth in August 1997.[1] In 1994, Czech astronomer Zdeněk Ceplecha reanalysed the data and suggested the passage would have reduced the asteroid's mass to about a third or half of its original mass, reducing its diameter to 2to.[4]

The object was tracked by military surveillance systems and sufficient data obtained to determine its orbit both before and after its 100-second passage through Earth's atmosphere. Its velocity was reduced by about 800m/s and the encounter significantly changed its orbital inclination from 15 degrees to 7 degrees.[5] If it had not entered at such a grazing angle, this meteoroid would have lost all its velocity in the upper atmosphere, possibly ending in an airburst, and any remnant would have fallen at terminal velocity.[6]

See also

Further reading

External links

Notes and References

  1. http://www.astrosociety.org/pubs/mercury/9806/impact.html Observation of Meteoroid Impacts by Space-Based Sensors
  2. Ceplecha . Z. . 1994 . Earth-grazing daylight fireball of August 10, 1972 . Astronomy and Astrophysics . 283 . 287 .
  3. Web site: NEO Chronology - NEO .
  4. https://web.archive.org/web/20050120051405/http://www.maa.agleia.de/Comet/Other/1972.html Daylight Fireball of August 10, 1972
  5. https://web.archive.org/web/20040307122520/http://www.fis.unipr.it/~albino/ITASN/GSNA/US19720810/US19720810.html US19720810 (Daylight Earth grazer)
  6. Robert Marcus, H. Jay Melosh, and Gareth Collins. Computing Effects of an Impact on Earth