A meteorite the size of a Volkswagen is not all that large, as these
things go. A 2004 model year Beetle (according to the VW website) is
161? long. That?s a little over 4 meters. Let?s assume your impactor
is a meteor with a diameter of 4 m. Iron meteors have a density of
about 8 gm/cm^3 or 8000 km/m^3. A 4-m diameter sphere has a volume of
33.5 m^3 (V=4/3*pi*r^3), and a mass of 268 metric tons (V*density; 1
metric ton = 1000kg).
An object this size enters the Earth?s atmosphere about every 3 years.
Objects this size do not make it to the Earth?s surface as an intact
body; they break up in the atmosphere into smaller chunks that cause
little or no damage at the surface. To get a chunk of the size you
are talking about to actually hit the Earth?s surface, you need to
start with a much larger body in space ? on the order of 30 meters
diameter. Objects of this size hit the Earth every couple hundred
years.
Assuming you start with something large enough to get a
Volkswagen-sized piece to hit the surface, one can use the on-line
crater-scaling calculator
(http://www.lpl.arizona.edu/tekton/crater_c.html) by Prof. Jay Melosh
at the Univ of AZ Lunar and Planetary Lab to calculate the diameter of
the crater that would result from the impact of this object. There
are a number of variables you can play with (e.g., the nature of the
target rock, the angle of impact, impact velocity, etc.), but for a
vertical impact onto unconsolidated sediments/soils, and an impact
velocity of 17 km/sec (typical for a non-cometary impact on Earth),
the resulting crater would have a final rim-to-rim diameter of about
400 meters. The impact would have release the energy equivalent of
9.25 kilotons of TNT (about half the Nagasaki or Hiroshima device
yields).
Jay also has an on-line calculator that will estimate the blast
effects as a function of distance from the impact point at
http://www.lpl.arizona.edu/impacteffects/. Most of the damage from an
impact this size is actually due to the air blast as the meteor
traverses the Earth?s atmosphere. A 30-meter initial diameter object
(about the size one would need to get chunks the size of a Volkswagen
hitting the surface) will break windows out to ~10 km from the impact
site, and wind speeds will briefly exceed hurricane force (~80mph); at
5 km, wood-frame buildings would collapse and most trees would be
blown down; at 1km, steel-frame building would be toast. There?s no
big fireball from this size impact, and ejecta is largely contained
within a few km radius.
An impact event of almost exactly this magnitude occurred about 25,000
to 50,000 years ago, just a bit south of your hypothetical impact.
The impact occurred in Odessa TX (about 300 miles south of the town of
Panhandle). There are numerous websites discussing the crater and the
impact. See:
http://www.utpb.edu/ceed/GeologicalResources/West_Texas_Geology/links/odessa_meteor.htm#top
http://www.alaska.net/~meteor/OTinfo.htm
http://www.tsha.utexas.edu/handbook/online/articles/view/MM/rym1.html
http://www.unb.ca/passc/ImpactDatabase/images/odessa.htm
http://www.texasbob.com/travel/tbt_odscrt.html
http://www.meteoritearticles.com/odessacraterarticle.html
As one might expect from my comments above, the Odessa meteor broke up
into several pieces upon entry, so there is actually a field of
smaller impact structures surrounding the main crater, which is
currently about 200 meters in diameter.
Pieces of the Odessa meteorite routinely sell for $1.00 to $2.00 per
gram on eBay. Bigger pieces are generally worth more per gram than
smaller ones.
For comparison, the Barringer Crater (aka "Meteor Crater") in Arizona,
was formed by the impact of a ~50-meter diameter chunk of iron
meteorite. The energy release in this impact was on the order of 18
megatons TNT. Impacts of this size occur every 2-4 thousand years.
The effects of an impact of this size are qualitatively different than
for the case you asked about; they produce a fireball that vaporizes
or melts a significant portion of the target rock, and the combined
thermal and blast effects are significantly more damaging. See
http://www.lpl.arizona.edu/SIC/impact_cratering/Enviropages/Barringer/barringerstartpage.html. |