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The Great Daylight 1972 Fireball
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The Great Daylight 1972 Fireball (or US19720810) is an Earth-grazing meteoroid which passed within 57 kilometres (35.4 miles) of the surface of the Earth at 20:29 UTC on August 10 1972. It entered the Earth's atmosphere 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.
ysis of its appearance and trajectory showed it was a meteoroid about (if a carbonaceous chondrite) to (if made of cometary ices) in diameter in the Apollo asteroid class in an Earth-crossing orbit that would make a subsequent close approach to Earth in August 1997.

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Encyclopedia
The Great Daylight 1972 Fireball (or US19720810) is an Earth-grazing meteoroid which passed within 57 kilometres (35.4 miles) of the surface of the Earth at 20:29 UTC on August 10 1972. It entered the Earth's atmosphere 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.
Description
Analysis of its appearance and trajectory showed it was a meteoroid about (if a carbonaceous chondrite) to (if made of cometary ices) in diameter in the Apollo asteroid class in an Earth-crossing orbit that would make a subsequent close approach to Earth in August 1997. In 1994, Czech astronomer Zdenek Ceplecha re-analysed the data and suggested the passage would have reduced the meteoroid's mass to about a third or half of its original mass (reducing its diameter to 2 to 10 metres).
The meteoroid's 100 second passage through the atmosphere reduced its velocity by about and the whole encounter significantly changed its orbital inclination from 15 degrees to 8 degrees.
The fireball was filmed by a tourist at the Grand Teton National Park in Wyoming using an 8-millimeter color movie camera.
What if it had collided?
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. Atmospheric entry of meteoroids is complex and a full calculation requires a full simulation, but a highly simplified calculation can be made using the web-based program by Collins et al.. This table shows how sensitive the result is to the entry angle and composition:
| Diameter | Density | Entry angle | Energy lost | Airburst altitude | Airburst energy |
|---|
| 3 | 3.4 | 1 degree | 1.3 kiloton | 43 km | 0.7 kiloton | | 3 | 3.4 | 45 degrees | 1.3 kiloton | 39 km | 0.4 kiloton | | 8 | 0.9 | 1 degree | 6 kiloton | 80 km | 0.4 kiloton | | 8 | 0.9 | 45 degrees | 6 kiloton | 45 km | 2 kiloton | |
All known Earth-grazing fireballs
Earth-grazing fireballs are a very rare kind of fireball caused by a meteoroid that collides with the Earth but survives the collision by passing through, and exiting, the atmosphere. four grazers have been scientifically observed.
- 1913-02-09, a narrow fireball stream led to conclusions a probable natural satellite of Earth had broken up
- 1972-08-10, US19720810 at 15 km/s above United States and Canada (first scientific observation)
- 1990-10-13, a 40 kilogram, 41.5 km per sec meteoroid passed at 97.9 km above Czechoslovakia
- 2006-03-29, fireball passed 18.8 km per sec through the atmosphere 71.4 km above Japan
- 2007-08-07, EN070807 passed through with an orbit belonging to the rare Aten asteroid type
See also
External links
- orbital characteristics from Global Superbolide Network Archive, 2000
- link to photos and cine film by Linda Baker
- youtube link to Linda Baker's film
- An other film on youtube
- overview of the event including photo by NASA's Astronomy Picture of the Day
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