Home | Contact Us | FAQ | Search & Site Map | Link to Us
Sign In | Join | Other 45 Sites in Network
Home
Discussion Groups
Biology
BiologyBotanyMicrobiologyEntomologyEvolutionPaleontology
Chemistry
General ChemistryAnalytical ChemistryElectrochemistryOrganic Synthesis
Earth Science
GeologyMineralogyOceanographyMeteorologyEarthquakes
Physics
General PhysicsResearchRelativityParticle PhysicsElectromagnetismFusionOpticsAcousticsNew Theories

Natural Science Forum / Biology / Paleontology / June 2007



Tip: Looking for answers? Try searching our database.

Ancient Meteor Blast May Have Caused Extinctions (Forwarded)

Thread view: 
Enable EMail Alerts  Start New Thread
Thread rating: 
mathematician - 10 Jun 2007 07:48 GMT
Hi,

I found an interesting article from sci.astro. Please take a look
for your comments.

It is quite unbelievable that so big meteorite (mentioned below text)
about 5 km in diameter had hit to the Earth about 13000 years ago
and possible caused "nuclear winter" ???

Best Regards,

Hannu

Newsgroups: sci.astro
Path:g2news1.google.com!news2.google.com!
newsfeed.stanford.edu!elk.ncren.net!newsflash.concordia.ca!news.sfu.ca!
utnut!utgpu!
utinfo!crux.astro.utoronto.ca!ayee
From: Andrew Yee <a...@crux.astro.utoronto.ca>
Subject: Ancient Meteor Blast May Have Caused Extinctions (Forwarded)
X-Nntp-Posting-Host: crux.astro.utoronto.ca
Content-Type: TEXT/PLAIN; charset=US-ASCII
Message-ID: <Pine.LNX.
4.30.0706071433190.19843-100000@crux.astro.utoronto.ca>
Sender: n...@campus-news-reading.utoronto.ca
Organization: UTCC Campus Access
Mime-Version: 1.0
Date: Thu, 7 Jun 2007 18:33:44 GMT

University of California-Santa Barbara

CONTACT
Gail Gallessich, 805-893-7220

FEATURED RESEARCHER
Luann Becker, 206-465-1005

May 23, 2007

Ancient Meteor Blast May Have Caused Extinctions, Report UC Santa
Barbara
Scientists

Santa Barbara, Calif. -- New scientific findings suggest that a large,
extraterrestrial rock may have exploded over North America 13,000
years
ago, explaining riddles that scientists have wrestled with for
decades,
including an abrupt cooling of the atmosphere and the extinction of
large
mammals.

Two scientists from the University of California, Santa Barbara
presented
the discovery today, along with two other researchers at a news
conference
at the annual meeting of the American Geophysical Union being held in
Acapulco, Mexico. Over 20 scientists contributed to the discovery.

James Kennett, paleoceanographer and professor emeritus in the
Department
of Earth Science at UC Santa Barbara, said that the discovery
potentially
explains three of the most-debated controversies of recent decades.

"This is what happens when you do interdisciplinary science," said
Luann
Becker, research scientist with UC Santa Barbara's Institute of
Crustal
Studies. "You can solve some of the bigger problems."

The time period in question is called the "Younger Dryas," a time of
abrupt cooling that lasted for about 1,000 years and occurred during
an
inter-glacial warm period. Evidence for the temperature change is
recorded
in ice cores.

According to the scientists, the extraterrestrial rock must have been
about five kilometers across, and either exploded in the atmosphere or
directly hit the Laurentide ice sheet located in the Northeastern
section
of North America. Wildfires across the continent would have resulted
from
the fiery impact, killing off the vegetation that was the food supply
of
many of the larger mammals like the woolly mammoths, causing them to
go
extinct. Since the Clovis people of North America hunted the mammoths
as a
major source of their food, they too were affected by the impact and
their
culture died out, explained Becker.

The scientific team visited over a dozen archaeological sites in North
America where they found high concentrations of iridium, an element
that
is rare on Earth, and is almost exclusively associated with meteors.
They
found microspherules of glass-like carbon, which form at high
temperatures
and are thought to be a result of the impact blast. Also present were
another type of impact tracer -- carbon molecules called fullerenes
with
gases trapped inside.

The team concluded that the impact of the space rock melted a large
portion of the Laurentide ice sheet, causing enormous amounts of cool,
fresh water to flow into the Atlantic and Arctic Oceans. This would
have
caused a major disruption of the circulation of warm and cold water in
these oceans, leading to a cooler atmosphere and the glaciation of the
Younger Dryas period.

The scientists found evidence for the impact as far west as the Santa
Barbara Channel Islands. Kennett said that the best examples from the
West
Coast were found at a site on Santa Rosa Island.

The Paleoclimate Program of the National Science Foundation and NASA
funded this research.
George - 10 Jun 2007 08:09 GMT
> Hi,
>
[quoted text clipped - 85 lines]
> go
> extinct.

Problem:  If it had struck an ice sheet that has been estimated to have
been as much as 8,000-10,000 feet thick, what forests existed that could
have caught fire?

George
mathematician - 11 Jun 2007 19:22 GMT
> > Hi,
>
[quoted text clipped - 91 lines]
>
> George

Yes, that is a problerm if meteorite is in question. What about
possibility
of icy comet of about 5 km in diameter ? Do any existing eveidences
support
this possibility ?

Hannu
George - 11 Jun 2007 22:27 GMT
>> > Hi,
>>
[quoted text clipped - 99 lines]
>
> Hannu

Same problem.  If it struck a 10,000 feet thick ice sheet, there are no
forests to catch fire, or else get destroyed.  On the other hand, the
amount of moisture released into the atmopshere would be huge.

George
Thomas T. Veldhouse - 12 Jun 2007 16:27 GMT
In sci.bio.paleontology George <george@yourservice.com> wrote:

> Same problem.  If it struck a 10,000 feet thick ice sheet, there are no
> forests to catch fire, or else get destroyed.  On the other hand, the
> amount of moisture released into the atmopshere would be huge.

I think the question related to the source of water being the comet rather
than the ice sheet.  Thus, the comet impacts forest and the meltwater from the
comment cools and dilutes the northern currents.

Signature

Thomas T. Veldhouse

If you took all of the grains of sand in the world, and lined
them up end to end in a row, you'd be working for the government!
               -- Mr. Interesting

George - 13 Jun 2007 02:46 GMT
> In sci.bio.paleontology George <george@yourservice.com> wrote:
>>
[quoted text clipped - 7 lines]
> from the
> comment cools and dilutes the northern currents.

Except that the suggestion was that it occurred up in Labrador, where there
was a 10,000 feet thick ice sheet at the time.  So there could hardly have
been a forest to get destroyed at that location.  That was the point I was
making.

George
mathematician - 13 Jun 2007 05:17 GMT
> > In sci.bio.paleontology George <geo...@yourservice.com> wrote:
>
[quoted text clipped - 21 lines]
>
> George

Could this climate change in Younger Dryas period be caused also by
solar variability, which could caused for example the break of
Laurentian (?)
ice-lake, if so then this meteorite/comet theory would not be
needed ?

I red in some Nature article that this climate change started
possible
in few tens of years  lasted about 1000 years, and also
ended few tens of years ?

Could the cause of this cold Younger Dryas period be changes in
sea currents ?

One changed sea current could be the Golf-stream, which definitely
would have influenced the climate conditions for example here in
Finland ?

Hannu
George - 13 Jun 2007 05:46 GMT
>> > In sci.bio.paleontology George <geo...@yourservice.com> wrote:
>>
[quoted text clipped - 45 lines]
>
> Hannu

Here is a link that discusses some of the ideas that have been bounced
around for what caused it, and possibly other similar periods.

http://en.wikipedia.org/wiki/Younger_Dryas

George
Matt - 13 Jun 2007 13:51 GMT
It's never been convincing to me that the early North American peoples
were the sole force behind a rapid extinction holocaust that took out
all the megafauna except the American bison.
Native peoples in Africa had hundreds of thousands of years to
multiply and to hunt game, where North Americans had only a couple of
thousand, and yet Africa is (or was, until modern large-scale poaching
and development) host to a very healthy collection of very large
mammals and their predators.
That there was an external cause like a comet assisting in the
destruction seems to me (an admitted non-expert) to be more plausible.

Matt Bille

> >> > In sci.bio.paleontology George <geo...@yourservice.com> wrote:
> >>
[quoted text clipped - 52 lines]
>
> George
mathematician - 20 Jun 2007 06:26 GMT
> >> > In sci.bio.paleontology George <geo...@yourservice.com> wrote:
>
[quoted text clipped - 52 lines]
>
> George

This is seems to be a good reference. You mention that there could
also be similar periods. I took a quick look at the picture which was
in your reference then I get following approximate similar periods:

http://en.wikipedia.org/wiki/Younger_Dryas

http://en.wikipedia.org/wiki/Image:Epica-vostok-grip-40kyr.png

37000-35500 years ago,
34500-33500 years ago,
33000-32000 years ago,
31500-28500 years ago,
28000-27000 years ago,
27000-14000 years ago,
13000-11500 years ago (approx. Younger Dryas period)

Causes of these could be possible: solar variability/ice-lake/sea
currents/possible comet or
asteroid impacts ???

I must read your reference and references in it more closely.

I remember that one possible origin of fractions of comets could be at
least those comets
which go too close to the Sun like the comet MacHoltz/P (if I
remembered the name right ?)
which could be fractioned due to too big gravitational forces near the
Sun. Orbits of these fragments
could then be expanding, maybe they are "collected" near the Jupiter
or into the asteroid belt
with Jupiter's pull force ???

Hannu
mathematician - 21 Jun 2007 17:24 GMT
> > "mathematician" <hapor...@luukku.com> wrote in message
>
[quoted text clipped - 90 lines]
>
> Hannu

Sorry that I did not rember to mention also an impotant matter
that on the million year time scale four periods of enhanced
VOLCANIC ACTIVITY have been identified in deep-sea core records,
of which two (in the middle Pliocene and middle Micoene epochs)
coincided with the beginning of glaciation in different parts
of the world.  (ref: The Cambridge Encyclopedia of Earth
Sciences, 1981,  pages 297-310, page. 305).

Hannu
Thomas T. Veldhouse - 13 Jun 2007 14:27 GMT
In sci.bio.paleontology George <george@yourservice.com> wrote:

> Except that the suggestion was that it occurred up in Labrador, where there
> was a 10,000 feet thick ice sheet at the time.  So there could hardly have
> been a forest to get destroyed at that location.  That was the point I was
> making.

Not during an interstitial warming period, as was noted in the article.

Signature

Thomas T. Veldhouse

Software is like sex; it's better when it's free.
       -- Linus Torvalds

George - 14 Jun 2007 02:56 GMT
> In sci.bio.paleontology George <george@yourservice.com> wrote:
>>
[quoted text clipped - 7 lines]
>
> Not during an interstitial warming period, as was noted in the article.

From the artricle:

"According to the scientists, the extraterrestrial rock must have been
about five kilometers across, and either exploded in the atmosphere or
directly hit the Laurentide ice sheet located in the Northeastern
section of North America."

So if it hit the ice sheet, again, what forest existed in the region could
have burned?

George
mathematician - 14 Jun 2007 17:29 GMT
> > In sci.bio.paleontology George <geo...@yourservice.com> wrote:
>
[quoted text clipped - 25 lines]
>
> George

If we think again the original meteorite theory mentined above,
then we have following estimates from which we can possibly see
that could this be possible at all in this case ?

I found one program which calculates possible crater diameter,
wood charred distance etc, if you give required parameters:

http://www.bumply.com/astro.html#5

A. If you give parameters: object's diameter = 5000 m, icey, strike
velocity = 20 km/s,
target density = 1000 kg/m3, you get the following results from the
calculator:

crater diameter = 54579 m, 1 st degree burns = 23292.35 km,
3 rd degree burns = 13054.85 km, wood charred = 9643.95 km,
white cotton ignites= 5208.3 km.

B. If you give parameters: object's diameter = 5000 m, icey, strike
velocity = 60 km/s,
target density = 1000 kg/m3, you get the following results from the
calculator:

crater diameter = 104157 m, 1 st degree burns = 69877.1 km,
3 rd degree burns = 39164.6 km, wood charred = 28931.85 km,
white cotton ignites= 15625 km.

Huge numbers, many of these distances are greater than diameter of the
Earth ?

Please try the calculator program with your parameters. What you got ?

Hannu
George - 15 Jun 2007 06:40 GMT
>> > In sci.bio.paleontology George <geo...@yourservice.com> wrote:
>>
[quoted text clipped - 62 lines]
>
> Hannu

I am very familiar with impact calculators.  I use the one on the
University of Arizona'a web site all the time.  But you are missing the
point here.  If it strikes a 10,000 feet thick ice sheet in a remote area,
there necessarily isn't going to be any forest that the resulting impact
can burn because the entire landscape is covered by ***a 10,000 feet thick
ice sheet***.

George
Bob Cain - 15 Jun 2007 08:48 GMT
> I am very familiar with impact calculators.  I use the one on the
> University of Arizona'a web site all the time.  But you are missing the
> point here.  If it strikes a 10,000 feet thick ice sheet in a remote area,
> there necessarily isn't going to be any forest that the resulting impact
> can burn because the entire landscape is covered by ***a 10,000 feet thick
> ice sheet***.

*Until* the object impacts.  Do you think that ice would stop that
size object from impacting whatever is beneath it with enough energy
left to splash magma all over the damn planet and start fires on the
other damn side of it?  Maybe it would only result in steam, as you
imply, but that's not what I saw on TV.  :-)

Bob
Signature


"Things should be described as simply as possible, but no simpler."

                                            A. Einstein

George - 15 Jun 2007 12:11 GMT
>> I am very familiar with impact calculators.  I use the one on the
>> University of Arizona'a web site all the time.  But you are missing the
[quoted text clipped - 12 lines]
>
> Bob

Umm, Bob (I can call you bob, right?).  You should take what you see on TV
with a grain of salt.

Using the University of Arizona's impact calculator and inputing data for a
5 km diameter bolide with a density of dense rock impacting (in this case,
water, since ice isn't available as a target in the impact calculator)
10,000 meters of water, for an observer 1,000 km away, here's what we get:

   Your Inputs:
   Distance from Impact: 1000.00 km = 621.00 miles
   Projectile Diameter: 5000.00 m = 16400.00 ft = 3.10 miles
   Projectile Density: 3000 kg/m3
   Impact Velocity: 11.00 km/s = 6.83 miles/s
   Impact Angle: 45 degrees
   Target Density: 1000 kg/m3
   Target Type: Liquid Water of depth 3048.00 meters, over typical rock.
   Energy:
   Energy before atmospheric entry: 1.19 x 1022 Joules = 2.84 x 106
MegaTons TNT
   The average interval between impacts of this size somewhere on Earth
during the last 4 billion years is 1.0 x 107years
   Major Global Changes:
   The Earth is not strongly disturbed by the impact and loses negligible
mass.
   The impact does not make a noticeable change in the Earth's rotation
period or the tilt of its axis.
   The impact does not shift the Earth's orbit noticeably.
   Crater Dimensions:
   What does this mean?

   The crater opened in the water has a diameter of 48.9 km = 30.3 miles

   For the crater formed in the seafloor:
   Transient Crater Diameter: 25.3 km = 15.7 miles
   Transient Crater Depth: 8.94 km = 5.55 miles

   Final Crater Diameter: 38.7 km = 24 miles
   Final Crater Depth: 0.889 km = 0.552 miles
 The crater formed is a complex crater.
 At this impact velocity ( < 12 km/s), little shock melting of the target
occurs.
   Thermal Radiation:
   What does this mean?

   At this impact velocity ( < 15 km/s), little vaporization occurs; no
fireball is created, therefore, there is no thermal radiation damage.
   Seismic Effects:
   What does this mean?

   The major seismic shaking will arrive at approximately 200 seconds.
   Richter Scale Magnitude: 8.7
   Mercalli Scale Intensity at a distance of 1000 km:

     III. Felt quite noticeably by persons indoors, especially on upper
floors of buildings. Many people do not recognize it as an earthquake.
Standing motor cars may rock slightly. Vibrations similar to the passing of
a truck.

     IV. Felt indoors by many, outdoors by few during the day. At night,
some awakened. Dishes, windows, doors disturbed; walls make cracking sound.
Sensation like heavy truck striking building. Standing motor cars rocked
noticeably.

   Ejecta:
   What does this mean?

   The ejecta will arrive approximately 494 seconds after the impact.
   At your position the ejecta arrives in scattered fragments
   Average Ejecta Thickness: 3.65 mm = 0.144 inches
   Mean Fragment Diameter: 570 micrometers = 22.4 1/1000 of an inch

   Air Blast:
   What does this mean?

   The air blast will arrive at approximately 3030 seconds.
   Peak Overpressure: 14900 Pa = 0.149 bars = 2.12 psi
   Max wind velocity: 33.2 m/s = 74.2 mph
   Sound Intensity: 83 dB (Loud as heavy traffic)
   Damage Description:

     Glass windows will shatter.

   So the impact doesn't spew hot lava all over the place since there is
no fireball (thus, no thermal radiation damage), and certainly if it struck
ice instead of water, the effects would likely be much less than this for
this distance.
George - 15 Jun 2007 12:12 GMT
>>> I am very familiar with impact calculators.  I use the one on the
>>> University of Arizona'a web site all the time.  But you are missing the
[quoted text clipped - 101 lines]
> struck ice instead of water, the effects would likely be much less than
> this for this distance.

Here is the link, try it:

http://www.lpl.arizona.edu/impacteffects/

George
mathematician - 15 Jun 2007 18:50 GMT
> >>> I am very familiar with impact calculators.  I use the one on the
> >>> University of Arizona'a web site all the time.  But you are missing the
[quoted text clipped - 107 lines]
>
> George

Yes OK, I took a quick look to the reference text (link to this paper
was found from your reference).

I have also found one present possible dangerous asteroid. Here are
references of it which I found:

Present situation in the Risk Page (many of these will be removed
when enough accurate measurements are available)

NeoDys Risk Page

http://newton.dm.unipi.it/cgi-bin/neodys/neoibo?riskpage:0;main

One present  example (diameter=0.270 km, H=19.7,  this is maybe
dangerous)

(99942) Apophis - impactor table
Object: 99942

    date        MJD      sigma sigimp   dist +/-   width
stretch    p_RE    exp. en.    PS
  YYYY/MM                               (RE)       (RE)      RE/
sig               MT
------------------------------------------------------------------------------------------------
2036/04/13.371 64796.371 -2.470 0.000    1.15 +/-    0.003  3.32E+03
2.07E-05  8.26E-03  -2.57
2042/04/13.720 66987.720 -2.494 0.000    1.41 +/-    0.000  1.12E+06
5.26E-08  2.10E-05  -5.24
2044/04/13.296 67718.296 -2.434 0.000    2.08 +/-    0.000  6.27E+05
3.57E-08  1.42E-05  -5.44
2069/04/13.078 76849.078  2.112 0.000    0.97 +/-    0.000  3.74E+05
4.41E-07  1.76E-04  -4.56
2069/10/15.971 77034.971  1.466 0.000    0.48 +/-    0.160  1.52E+06
3.81E-07  1.52E-04  -4.63
2072/10/15.333 78130.333 -3.870 0.000    0.48 +/-    0.089  6.09E+06
1.57E-10  6.26E-08  -8.03
2076/07/30.873 79514.873  2.720 1.214   34.89 +/-   26.902  1.49E+07
3.73E-11  1.44E-08  -8.69

Based on 1000 optical observations (of which   5 are rejected as
outliers)
from 2004/03/15.108 to 2006/08/16.627, and also on seven radar data
points
on 2005/01/27, 2005/01/29, 2005/01/31, 2005/08/07 and 2006/05/06.

Coordinates are given on the Target Plane
Unit is one Earth radius, but impact cross section
has radius between  2.15 and  2.16 Earth radii

http://newton.dm.unipi.it/cgi-bin/neodys/neoibo?objects:Apophis;main
http://newton.dm.unipi.it/cgi-bin/neodys/neoibo?objects:Apophis;statpts;gif
http://newton.dm.unipi.it/cgi-bin/neodys/neoibo?objects:Apophis;properel;gif
http://earn.dlr.de/nea/099942.htm
http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=99942;orb=1   (simulation of the
orbit,
possible impact velocity can be esitimated from this ?)

Conversion of Absolute Magnitude (H) to Diameter

http://cfa-www.harvard.edu/iau/lists/Sizes.html

This is quite inaccurate method  to estimate diameters, but it is only
available method ?

Hannu
George - 15 Jun 2007 19:01 GMT
>> >>> I am very familiar with impact calculators.  I use the one on the
>> >>> University of Arizona'a web site all the time.  But you are missing
[quoted text clipped - 190 lines]
>
> Hannu

As of August 5, 2006, the threat level for Apophis had been reduced to
level 0.  As for your question about estimating diameters, I don't have a
good answer for you at this time.  I'll check back with you if I figure one
out.

George
mathematician - 16 Jun 2007 12:31 GMT
> >> "George" <geo...@yourservice.com> wrote in message
>
[quoted text clipped - 201 lines]
>
> George

I roughly estimated the velocity difference of Apophis and Earth (they
are orbiting same direction quite close each others as we see in the
simulation pictures referenced above) and I got that possible
impact velosity would be about 1 km/s, if I calculated right ?

The exact diamenter is little uncertain and there was an earlier
estimation of H which was H=19.20, which gave range
430 m-970 m (http://earn.dlr.de/nea/99942.htm, printed 19.8.2005),
but present estimation is 270 m ?

How big tsunamis would this cause if it would hit in some ocean ?

Hannu
George - 16 Jun 2007 20:34 GMT
>> >> "George" <geo...@yourservice.com> wrote in message
>>
[quoted text clipped - 234 lines]
>
> Hannu

According to the impact calculator, if the object is 270 meters in
diameter, and consists of dense rock, and is traveling at 1 km/s at a 45
degree angle relative to the earth's surface, it will break up in the
atmosphere at an altitude of 28,200 ft.  If the object is 439 meters in
diameter, then using the same parameters as before, the object will break
up in the atmosphere at an altitude of 28,400 ft, which is an odd result.
Using a diameter of 970 meters, the object would break up at 28,500 ft,
again, an odd result.  Obviously, either the program has some errors in the
calculations, or else there is a minimum size and density required before
an object will strike the earth, which I think is highly likely.  That
said, if such an object exploded over a densely populated area, it would be
devastating, to say the least.

George
mathematician - 19 Jun 2007 06:12 GMT
> >> "mathematician" <hapor...@luukku.com> wrote in message
>
[quoted text clipped - 250 lines]
>
> read more ?

A. It would then be like "a shot with a shotgun" (v = about 1km/s, hit
angle to the Earth's
atmosphere = more close to 90 than 45 ?), many fragments of different
sizes results ?

How do we know that there is no big iron fragments included in the
structure of Apophis ?

If I remember right there was also some fragmented iron (?) meteorite
which hit to
Estonia about 2400 years ago (there was a TV-program some time ago
about
this in finnish TV) ?

I just think that could these meteorites about 13000 years ago, about
2400 years ago
and Apophis have anything properties in common ?

B. I found an abstract from the net about determination of H (and also
diameter) of Apophis:

( http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=998112
)

---COPY BELOW-----
Proceedings of the International Astronomical Union (2007), 2: 451-454
Cambridge University Press
doi:10.1017/S1743921307003560
Published online by Cambridge University Press 03May2007

Contributed Papers
Albedo and size of (99942) Apophis from polarimetric observations?
Alberto Cellinoa1, Marco Delb?a1a2 and Edward F. Tedescoa3

a1 INAF-Osservatorio Astronomico di Torino, strada Osservatorio 20,
10025 Pino Torinese, Italy email: cellino@inaf.oato.it
a2 Observatoire de la C?te d'Azur, BP 229, Nice, France email:
delbo@obs-nice.fr
a3 University of New Hampshire, USA email: Ed.Tedesco@unh.edu

Abstract.

We have obtained the first accurate determination of the albedo of
(99942) Apophis, by means of polarimetric observations carried out at
the VLT. The observations allowed us to obtain the slope of the
polarization-phase curve of this object, from which an albedo estimate
of 0.33 ? 0.04 could be obtained. From our observations we also
obtained a new estimate of the absolute magnitude: H = 19.7 ? 0.2
(assuming G=0.25, which applies to S- and Q-type asteroids). Based on
these results, we derive for the size of Apophis a value of 270 ? 30
meters. The accuracy of this size estimate is mostly related to
uncertainties in H, whereas the obtained albedo value should be
considered more robust. Our observations convincingly show that
polarimetry is an effective and efficient tool to obtain accurate
albedos and sizes for small and faint potentially hazardous asteroids.

Key Words: Asteroids; polarization

Footnotes
? Based on observations obtained at the European Southern Observatory
(ESO), DDT request 276.C-5030
---COPY ABOVE-----

http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=998112

Hannu
Thomas T. Veldhouse - 19 Jun 2007 13:57 GMT
In sci.bio.paleontology mathematician <haporopu@luukku.com> wrote:

Sheesh ... care to post edit next time?  You don't have to post ALL the
previous text with each post.

Signature

Thomas T. Veldhouse

Software is like sex; it's better when it's free.
       -- Linus Torvalds

mathematician - 19 Jun 2007 17:42 GMT
To George:

A. It would then be like "a shot with a shotgun" (v = about 1km/s, hit
angle to the Earth's atmosphere = between 0 to 90 (45 is average
estimate ?)),
many fragments of different sizes results ?

How do we know that there is no big iron fragments included in the
structure of Apophis which could possible cause tsunamis if hit into
ocean?

If I remember right there was also some fragmented iron (?) meteorite
which hit to Estonia about 2400 years ago (there was a TV-program
some time ago about this in finnish TV) ?

I just think that could these meteorites about 13000 years ago, about
2400 years ago and Apophis have anything properties in common
(and maybe there exist also other possible years ) ???

I found one interesting reference (possible could be related to this
phenomena if enough properties in common exists ???) but
unfortunately I don't have that paper on my hands now:

Kerr, R. A., 1992.
Earth Gains a Retinue of Mini Asteroids.
Science, vol. 258, no. 5081, Oct 16, p. 403.

I must read this in the library. I comment it later if I find it.

B. I found an abstract from the net about determination of H (and also
diameter) of Apophis:

http://journals.cambridge.org/action/displayAbstract?fromPage=online&...

--COPY BELOW-----
Proceedings of the International Astronomical Union (2007), 2: 451-454
Cambridge University Press
doi:10.1017/S1743921307003560
Published online by Cambridge University Press 03May2007

Contributed Papers
Albedo and size of (99942) Apophis from polarimetric observations†
Alberto Cellinoa1, Marco Delbòa1a2 and Edward F. Tedescoa3

a1 INAF-Osservatorio Astronomico di Torino, strada Osservatorio 20,
10025 Pino Torinese, Italy email: cell...@inaf.oato.it
a2 Observatoire de la Côte d'Azur, BP 229, Nice, France email:
d...@obs-nice.fr
a3 University of New Hampshire, USA email: Ed.Tede...@unh.edu

Abstract.

We have obtained the first accurate determination of the albedo of
(99942) Apophis, by means of polarimetric observations carried out at
the VLT. The observations allowed us to obtain the slope of the
polarization-phase curve of this object, from which an albedo estimate
of 0.33 ± 0.04 could be obtained. From our observations we also
obtained a new estimate of the absolute magnitude: H = 19.7 ± 0.2
(assuming G=0.25, which applies to S- and Q-type asteroids). Based on
these results, we derive for the size of Apophis a value of 270 ± 30
meters. The accuracy of this size estimate is mostly related to
uncertainties in H, whereas the obtained albedo value should be
considered more robust. Our observations convincingly show that
polarimetry is an effective and efficient tool to obtain accurate
albedos and sizes for small and faint potentially hazardous asteroids.

Key Words: Asteroids; polarization

Footnotes
† Based on observations obtained at the European Southern Observatory
(ESO), DDT request 276.C-5030
---COPY ABOVE-----

http://journals.cambridge.org/action/displayAbstract?fromPage=online&...

Hannu

(I'am sorry about I did not notice long reply texts
which google generated automatically. They are quite
annoying.)
Hannu Poropudas - 19 Jun 2007 18:06 GMT
I found one discussion in the the of this article
(Kerr, R. A., 1992.
Earth Gains a Retinue of Mini Asteroids.
Science, vol. 258, no. 5081, Oct 16, p. 403. )

----Partly COPIED BELOW------

From: jsco...@lpl.arizona.edu (Jim Scotti x2717)
Newsgroups: sci.astro,sci.space
Subject: Re: "Earth Gains a Retinue of Mini-Asteroids"
Message-ID: <1992Oct31.075547.28204@organpipe.uug.arizona.edu>
Date: 31 Oct 92 07:55:47 GMT
References: <1992Oct29.170729.20363@cs.rochester.edu>
Sender: n...@organpipe.uug.arizona.edu
Distribution: na
Organization: Lunar & Planetary Laboratory, Tucson AZ.
Lines: 66

In article <1992Oct29.170729.20...@cs.rochester.edu>
d...@cs.rochester.edu (Paul Dietz) writes:
>Science (10/16/92, page 403), reports that Gehrels and colleagues in
>the Spacewatch program have detected 8 very near earth asteroids over
[quoted text clipped - 7 lines]
>body, and such events were calculated to occur once every 2 to 3
>centuries, something is screwy here.

Not really screwy.  The number of 50 meter objects is enhanced by
about 10 times and the Tunguska type events probably happen once
or a few times per century.  Remember, 3 out of 4 enter over water
and may be less likely to be detected.  Also, perhaps a large
fraction of them disintegrate higher in the atmoshpere, causing
a much smaller disturbance in the lower atmosphere than that of
the Tunguska event.  Also, the best guess I've heard for the size
of the Tunguska progenitor is between 50 and 100 meters.  The 10
meter sized objects are enhanced by a factor of 100 and the trend
from the larger objects to the smallest is a gradual transition
that starts at around 100 meters size.

>The orbits of the bodies are unexpectedly similar to Earth's.
>Two have orbits more like earth's than any known body; one was that
>asteroid that was mistaken for a spent rocket body.

Also known as 1991 VG.

>These couldn't be Frank's minicomets, could they?  His putative
>objects are supposedly in prograde, earth-like orbits, to reduce the
>impact velocity enough to avoid observational constraints.

Frank's minicomets were estimated to be 10-30 meters in size.  The
number of objects in this size that he estimated to account for
what was probably detector noise was at least a million times the
the number extrapolated from the larger Near Earth asteroid population
and therefore is a population at least 10,000 times more numerous
than
what has now been found by Spacewatch.  In short, with our
sensitivity,
we should see at least 1000 of Frank's minicomets each NIGHT!!!!!!  I
think the Spacewatch survey has now effectively disproven Frank's
hypothesis used to explain his so called "atmospheric holes".

Incidentally, an earlier CCD developed by Spacewatch in the
early 1980's (an old RCA 320x512 chip) was used by a colleague
of Frank's from JPL to survey for the minicomets directly.  This
investigator claimed to have detected at least one such object
on two consecutive images.  Without consulting the Spacewtach
crew, he announced his "discovery".  When we were finally able
to look at his images, we concluded that what he was looking
at was detector noise!

>    Paul F. Dietz
>    d...@cs.rochester.edu

Jim.
---------------------------------------------
Jim Scotti
{jsco...@lpl.arizona.edu}
Lunar & Planetary Laboratory
University of Arizona
Tucson, AZ 85721 USA

From: jsco...@lpl.arizona.edu (Jim Scotti x2717)
Newsgroups: sci.space
Subject: Re: "Earth Gains a Retinue of Mini-Asteroids"
Message-ID: <1992Nov4.204744.15077@organpipe.uug.arizona.edu>
Date: 4 Nov 92 20:47:44 GMT
References: <Bx3CM5.7Gx.1@cs.cmu.edu>
Sender: n...@organpipe.uug.arizona.edu
Distribution: sci
Organization: Lunar & Planetary Laboratory, Tucson AZ.
Lines: 62

In article <Bx3CM5.7G...@cs.cmu.edu> a...@elegabalus.cs.qub.ac.uk
writes:
{Actually, I (jsco...@lpl.arizona.edu) wrote this:}
>> Not really screwy.  The number of 50 meter objects is enhanced by
>> about 10 times and the Tunguska type events probably happen once
[quoted text clipped - 5 lines]
>late 70's - early 80's? It was never connected to any source that I
>am aware of.

I vaguely remember hearing something about this.  The rate of small
asteroid impact could very well account for such an event.  I doubt
we can conclusively identify it as an asteroid impact, but the
probability of such an event happening is quite high.

>Some theorized it was caused by an undersea volcanic explosion, but
>no one succeeded in associating it with one. It was not a nuclear
>explosion, although some at first suggested that. It is unlikely to
>have been a non-nuclear explosion, ie no ships disappeared and I'm
>not sure I see a motive for an experimental blast in that part of the
>world.

In the absence of further evidence, we'll just have to add small
asteroid impacts as a possibility.

>Just a thought, although I would not expect a mushroom cloud from
>such a comet strike. I'm not sure I can even see a mechanism for
>creating one from a Tunguska class strike.

The mechanism is quite understandable.  You have an object moving
at hypersonic velocity as it enters the atmosphere.  A stony or
stony iron object could easily survive into the low atmosphere where
the aerodynamical stress catastrophically ruptures it and it explodes
just like a bomb.  The estimated impact energies of 10-100 meter
objects traveling at typical velocities is measured in the kilotons
on the small end to 10s of megatons on the large end and that kinetic
energy has to go somewhere!  Smaller objects fracture high in the
atmosphere and appear as bright bolides which leave trails and
fragments along the way.  If the object is strong enough, it might
survive largely intact with most of its kinetic energy and might
create an impact crater such as was made about 50,000 years ago when
the Diablo Canyon Meteor crater was formed in Arizona.  That crater
is thought to have been formed by the impact of a stony iron object
only about 30 meters in diameter.  Objects strong enough to survive
atmospheric entry are fortunately rare.

By the way, the Tuguska event was observed by residents of the
region and their description of the explosion matchs that of a nuclear
bomb blast quite closely.

Jim.
---------------------------------------------
Jim Scotti
{jsco...@lpl.arizona.edu}
Lunar & Planetary Laboratory
University of Arizona
Tucson, AZ 85721 USA
---------------------------------------------

From: jsco...@lpl.arizona.edu (Jim Scotti x2717)
Newsgroups: sci.astro,sci.space
Subject: Re: "Earth Gains a Retinue of Mini-Asteroids"
Message-ID: <1992Nov7.011656.14470@organpipe.uug.arizona.edu>
Date: 7 Nov 92 01:16:56 GMT
References: <1992Oct29.170729.20363@cs.rochester.edu>
<1992Oct31.075547.28204@organpipe.uug.arizona.edu>
<BxACCF.D3A@techbook.com>
Sender: n...@organpipe.uug.arizona.edu
Distribution: na
Organization: Lunar & Planetary Laboratory, Tucson AZ.
Lines: 44

In article <BxACCF....@techbook.com> d...@techbook.com (Dan Tilque)
writes:
>jsco...@lpl.arizona.edu (Jim Scotti x2717) writes:
>>d...@cs.rochester.edu (Paul Dietz) writes:
[quoted text clipped - 14 lines]
>
>Anyone know about this?

Yup, I do.  You are remembering the meteorite fall called "Sikhote-
Alin"
which happened in 1947 in Siberia.  The fall created about 200 small
craters of the non-explosive type created by the fall of large
objects
traveling relatively slowly, perhaps at terminal velocity.  The
largest
crater was about 26.5 meters in diameter.  I think that about 50 tons
of
material was recovered and the progenitor was estimated as being
about
200 tons before atmospheric entry.  I suppose the object would have
been
around 5 meters diameter before entry and was probably a stoney iron.

This size object probably hits the Earth around 10 times per year and
I suppose about 1% of them are stoney iron, so a fall of this type
probably happens on the order of once a decade.

>---
>Dan Tilque    --     d...@techbook.com

Jim.
---------------------------------------------
Jim Scotti
{jsco...@lpl.arizona.edu}
Lunar & Planetary Laboratory
University of Arizona
Tucson, AZ 85721 USA
---------------------------------------------

----COPY ABOVE--------------------

Hannu
Bob Cain - 18 Jun 2007 04:07 GMT
>> *Until* the object impacts.  Do you think that ice would stop that
>> size object from impacting whatever is beneath it with enough energy
[quoted text clipped - 5 lines]
>
> Umm, Bob (I can call you bob, right?).  

Sure.

> You should take what you see on TV
> with a grain of salt.

:-)  Just didn't want you to think I thought I knew what I was talking
about.

>     So the impact doesn't spew hot lava all over the place since there is
> no fireball (thus, no thermal radiation damage), and certainly if it struck
> ice instead of water, the effects would likely be much less than this for
> this distance.

Thanks.  The one that wiped out the dinosaurs was the one I saw
reported on a TV show and the simulation showed molten stuff splashing
thousands of miles up into North America lighting fires all over hell
and back.  Bad science reporting or a much bigger event?

Bob
Signature


"Things should be described as simply as possible, but no simpler."

                                            A. Einstein

George - 18 Jun 2007 11:00 GMT
>>> *Until* the object impacts.  Do you think that ice would stop that
>>> size object from impacting whatever is beneath it with enough energy
[quoted text clipped - 28 lines]
>
> Bob

Probably both.

George
 
Sign In
Join
My Latest Posts
My Monitored Threads
My Blog
My Photo Gallery
My Profile
My Homepage

Start New Thread
Enable EMail Alerts
Rate this Thread



©2009 Advenet LLC   Privacy Policy - Terms of Use
This website includes both content owned or controlled by Advenet as well as content owned or controlled by third parties.