Re: [meteorite-list] Meteor Crater Shape and Entry Angle

2010-09-10 Thread David Norton
How about SW to NE? I believe there are several finds along that path that
match the Canyon Diablo material.

-Original Message-
From: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of Meteorites
USA
Sent: Friday, September 10, 2010 10:38 AM
To: meteorite-list@meteoritecentral.com
Subject: Re: [meteorite-list] Meteor Crater Shape and Entry Angle

Hi John, Thanks for the details. It's interesting to note that the angle 
of descent is not known, though there are educated guesses or 
calculations. What can probably be agreed is that an impactor with an 
entry angle of 45* degrees could produce a round crater. Meaning of 
course that Meteor Crater, since it's not perfectly round as evidenced 
by the "bulges" in the NW and SE corners, must have been produced by an 
impactor with a trajectory much shallower than 45 degrees. Logically.

Here's another question. Which direction was it traveling SE to NW or NW 
to SE?

According to the Shoemaker paper here: 
http://arrowsmith410-598.asu.edu/Lectures/Lecture16/i0-8137-5402-X-2-0-399Sh
oemaker.pdf

"...Somewhat greater energy was
required if the projectile struck at an oblique angle, as suggested
by the presence of faults with underthrust displacement on the
north and west walls of Meteor Crater"

It suggests a NW direction of travel... is this correct? And how do we know?

Does the "underthrust displacement" imply that the impactor was 
traveling from the SE toward the NW?

Eric



On 9/10/2010 8:05 AM, Kashuba wrote:
> Eric, Bernd, Sterling, List,
>
> David Kring of LPL put together a great guidebook for the 2007 MetSoc tour
> of the crater (150 pages).  He is Gene Shoemakers successor as advisor to
> the Barringer family.  He and family members lead the tour.  Carolyn
> Shoemaker was there too.
>
> Chapter 9. "Trajectory" begins and ends thusly:
>
> The trajectory of the impacting asteroid is another issue of considerable
> debate and still unresolved.
> Historically, circular plan views of impact craters confounded many
> investigators who assumed a circular
> crater requires a vertical impact. They wondered why more craters are not
> elliptical. Gilbert and
> Barringer both realized that 45 degree impacts are the most probable
> trajectories for meteoritic material.
> Yet Gilbert, like many of his contemporaries, mistakenly thought a 45
degree
> impact produces an oval
> crater (Hoyt, 1987). Barringer, on the other hand, realized that a 45
degree
> impact will produce a round
> crater (Hoyt, 1987). Despite this insight, Barringer, like Gilbert,
> initially assumed that the northern
> Arizona impact had been vertical or nearly vertical and that the asteroid
> was buried beneath the center of
> the crater floor.
>
> When extensive drilling did not locate a main mass beneath the crater
floor
> and instead only
> produced traces of the projectile, Barringer began to consider other
> options. He had already noted several
> features that seem to have a directional symmetry.
>
> - snip -
>
> More recently, techniques similar to those of Sutton were applied by
> Holliday et al. (2005) to the
> Odessa impact site. They estimated the Odessa craters were produced
> approximately 63,000 years ago.
> Although the ages of Barringer and Odessa craters are still not precisely
> known, these approximate ages
> suggest Odessa formed earlier, with the caveat that the Barringer crater
may
> be older than 49,000 yrs.
> (See discussion in Chapter 11). Thus, the two impact events may not be
> directly related and may not have
> any bearing on the issue of trajectory.
>
> Nonetheless, several other potential indicators of trajectory survive (and
> even the Odessa connection
> might be revived). Unfortunately, these indicators cannot be reconciled at
> the present time and I think it
> fair to conclude that the trajectory of the impacting asteroid that
produced
> Barringer Crater remains
> uncertain.
>
> Chapter 9:
>
http://www.lpi.usra.edu/publications/books/barringer_crater_guidebook/chapte
> r_9.pdf
>
> Whole "guidebook":
>
http://www.lpi.usra.edu/publications/books/barringer_crater_guidebook/index.
> shtml
>
>
> Regards,
>
> - John
>
> Ontario, California
>
>
> -----Original Message-----
> From: meteorite-list-boun...@meteoritecentral.com
> [mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of
> bernd.pa...@paulinet.de
> Sent: Friday, September 10, 2010 3:26 AM
> To: Meteorite-list@meteoritecentral.com
> Subject: [meteorite-list] Meteor Crater Shape and Entry Angle
>
> Eric wrote:
>
> "The crater is not perfectly round as would be expected from an impactor
> coming in at a sharper an

Re: [meteorite-list] Meteor Crater Shape and Entry Angle

2010-09-10 Thread Chris Peterson
Not at all logically. Meteor Crater was round after the impact. Its current 
shape is produced by the non-isotropic nature of the local geology. In 
essence, it has eroded into its current shape. This process is well 
understood. There is no evidence at all that the impactor arrived at a 
shallow enough angle to actually produce an oval crater.


With our current crater analysis skills, I'd say any suggestion of a 
specific impact angle or direction is scarcely better than a pure guess. And 
even the reports estimating mass and velocity I view with a high degree of 
skepticism.


Chris

*
Chris L Peterson
Cloudbait Observatory
http://www.cloudbait.com


- Original Message - 
From: "Meteorites USA" 

To: 
Sent: Friday, September 10, 2010 11:37 AM
Subject: Re: [meteorite-list] Meteor Crater Shape and Entry Angle


Hi John, Thanks for the details. It's interesting to note that the angle 
of descent is not known, though there are educated guesses or 
calculations. What can probably be agreed is that an impactor with an 
entry angle of 45* degrees could produce a round crater. Meaning of course 
that Meteor Crater, since it's not perfectly round as evidenced by the 
"bulges" in the NW and SE corners, must have been produced by an impactor 
with a trajectory much shallower than 45 degrees. Logically.


Here's another question. Which direction was it traveling SE to NW or NW 
to SE?


According to the Shoemaker paper here: 
http://arrowsmith410-598.asu.edu/Lectures/Lecture16/i0-8137-5402-X-2-0-399Shoemaker.pdf


"...Somewhat greater energy was
required if the projectile struck at an oblique angle, as suggested
by the presence of faults with underthrust displacement on the
north and west walls of Meteor Crater"

It suggests a NW direction of travel... is this correct? And how do we 
know?


Does the "underthrust displacement" imply that the impactor was traveling 
from the SE toward the NW?


Eric


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Re: [meteorite-list] Meteor Crater Shape and Entry Angle

2010-09-10 Thread GeoZay


>>What can probably be agreed is  that an impactor with an 
entry angle of 45* degrees could produce a round  crater. Meaning of 
course that Meteor Crater, since it's not perfectly round  as evidenced 
by the "bulges" in the NW and SE corners, must have been  produced by an 
impactor with a trajectory much shallower than 45 degrees.  Logically.<<

I don't know, but I wonder if the shape of the terrain  upon 
impact(hills/gulleys etc) or perhaps a varied pattern of rock strength  
underground could 
have had some influence to the craters shape?
GeoZay  

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Re: [meteorite-list] Meteor Crater Shape and Entry Angle

2010-09-10 Thread Meteorites USA
Hi John, Thanks for the details. It's interesting to note that the angle 
of descent is not known, though there are educated guesses or 
calculations. What can probably be agreed is that an impactor with an 
entry angle of 45* degrees could produce a round crater. Meaning of 
course that Meteor Crater, since it's not perfectly round as evidenced 
by the "bulges" in the NW and SE corners, must have been produced by an 
impactor with a trajectory much shallower than 45 degrees. Logically.


Here's another question. Which direction was it traveling SE to NW or NW 
to SE?


According to the Shoemaker paper here: 
http://arrowsmith410-598.asu.edu/Lectures/Lecture16/i0-8137-5402-X-2-0-399Shoemaker.pdf


"...Somewhat greater energy was
required if the projectile struck at an oblique angle, as suggested
by the presence of faults with underthrust displacement on the
north and west walls of Meteor Crater"

It suggests a NW direction of travel... is this correct? And how do we know?

Does the "underthrust displacement" imply that the impactor was 
traveling from the SE toward the NW?


Eric



On 9/10/2010 8:05 AM, Kashuba wrote:

Eric, Bernd, Sterling, List,

David Kring of LPL put together a great guidebook for the 2007 MetSoc tour
of the crater (150 pages).  He is Gene Shoemakers successor as advisor to
the Barringer family.  He and family members lead the tour.  Carolyn
Shoemaker was there too.

Chapter 9. "Trajectory" begins and ends thusly:

The trajectory of the impacting asteroid is another issue of considerable
debate and still unresolved.
Historically, circular plan views of impact craters confounded many
investigators who assumed a circular
crater requires a vertical impact. They wondered why more craters are not
elliptical. Gilbert and
Barringer both realized that 45 degree impacts are the most probable
trajectories for meteoritic material.
Yet Gilbert, like many of his contemporaries, mistakenly thought a 45 degree
impact produces an oval
crater (Hoyt, 1987). Barringer, on the other hand, realized that a 45 degree
impact will produce a round
crater (Hoyt, 1987). Despite this insight, Barringer, like Gilbert,
initially assumed that the northern
Arizona impact had been vertical or nearly vertical and that the asteroid
was buried beneath the center of
the crater floor.

When extensive drilling did not locate a main mass beneath the crater floor
and instead only
produced traces of the projectile, Barringer began to consider other
options. He had already noted several
features that seem to have a directional symmetry.

- snip -

More recently, techniques similar to those of Sutton were applied by
Holliday et al. (2005) to the
Odessa impact site. They estimated the Odessa craters were produced
approximately 63,000 years ago.
Although the ages of Barringer and Odessa craters are still not precisely
known, these approximate ages
suggest Odessa formed earlier, with the caveat that the Barringer crater may
be older than 49,000 yrs.
(See discussion in Chapter 11). Thus, the two impact events may not be
directly related and may not have
any bearing on the issue of trajectory.

Nonetheless, several other potential indicators of trajectory survive (and
even the Odessa connection
might be revived). Unfortunately, these indicators cannot be reconciled at
the present time and I think it
fair to conclude that the trajectory of the impacting asteroid that produced
Barringer Crater remains
uncertain.

Chapter 9:
http://www.lpi.usra.edu/publications/books/barringer_crater_guidebook/chapte
r_9.pdf

Whole "guidebook":
http://www.lpi.usra.edu/publications/books/barringer_crater_guidebook/index.
shtml


Regards,

- John

Ontario, California


-Original Message-
From: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of
bernd.pa...@paulinet.de
Sent: Friday, September 10, 2010 3:26 AM
To: Meteorite-list@meteoritecentral.com
Subject: [meteorite-list] Meteor Crater Shape and Entry Angle

Eric wrote:

"The crater is not perfectly round as would be expected from an impactor
coming in at a sharper angle. In fact the crater is more elliptical in
shape."

SHOEMAKER E.M. and KIEFFER S.W. (1974, 1979) Guidebook to the
Geology of Meteor Crater, Arizona (Publ. No. 17, Center for Meteorite
Studies, Arizona State University, Tempe, Arizona):

"Regional jointing has controlled the shape of the crater, which is somewhat
squarish in outline; the diagonals of the "square" coincide with the trend
of the
two main sets of joints. The largest tears occur in the "corners" of the
crater."

Eric also inquired:

"What would a "relatively low" impact angle be? 10 degrees, 20 degrees?"

I tried to find more precise information on that but was unable to find
something
that might be of help here. Maybe someone else can shed more light on this!

Regards,

Bernd

__

Re: [meteorite-list] Meteor Crater Shape and Entry Angle

2010-09-10 Thread Richard Kowalski
To produce an elongated crater you need a very low angle impact, on the order 
of only a few degrees at most.

Here's a quick, but more detailed answer. Additional searches will allow reader 
to find explanations with as much detail (and math) as they would like.

http://www.scientificamerican.com/article.cfm?id=why-are-impact-craters-al

--
Richard Kowalski
Full Moon Photography
IMCA #1081


--- On Fri, 9/10/10, bernd.pa...@paulinet.de  wrote:

> From: bernd.pa...@paulinet.de 
> Subject: [meteorite-list] Meteor Crater Shape and Entry Angle
> To: Meteorite-list@meteoritecentral.com
> Date: Friday, September 10, 2010, 3:25 AM
> Eric wrote:
> 
> "The crater is not perfectly round as would be expected
> from an impactor 
> coming in at a sharper angle. In fact the crater is more
> elliptical in shape."
> 
> SHOEMAKER E.M. and KIEFFER S.W. (1974, 1979) Guidebook to
> the
> Geology of Meteor Crater, Arizona (Publ. No. 17, Center for
> Meteorite
> Studies, Arizona State University, Tempe, Arizona):
> 
> "Regional jointing has controlled the shape of the crater,
> which is somewhat
> squarish in outline; the diagonals of the "square" coincide
> with the trend of the
> two main sets of joints. The largest tears occur in the
> "corners" of the crater."
> 
> Eric also inquired:
> 
> "What would a "relatively low" impact angle be? 10 degrees,
> 20 degrees?"
> 
> I tried to find more precise information on that but was
> unable to find something
> that might be of help here. Maybe someone else can shed
> more light on this!
> 
> Regards,
> 
> Bernd
> 
> __
> Visit the Archives at 
> http://www.meteoritecentral.com/mailing-list-archives.html
> Meteorite-list mailing list
> Meteorite-list@meteoritecentral.com
> http://six.pairlist.net/mailman/listinfo/meteorite-list
> 


  

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Re: [meteorite-list] Meteor Crater Shape and Entry Angle

2010-09-10 Thread Kashuba
Eric, Bernd, Sterling, List,

David Kring of LPL put together a great guidebook for the 2007 MetSoc tour
of the crater (150 pages).  He is Gene Shoemakers successor as advisor to
the Barringer family.  He and family members lead the tour.  Carolyn
Shoemaker was there too.  

Chapter 9. "Trajectory" begins and ends thusly:

The trajectory of the impacting asteroid is another issue of considerable
debate and still unresolved.
Historically, circular plan views of impact craters confounded many
investigators who assumed a circular
crater requires a vertical impact. They wondered why more craters are not
elliptical. Gilbert and
Barringer both realized that 45 degree impacts are the most probable
trajectories for meteoritic material.
Yet Gilbert, like many of his contemporaries, mistakenly thought a 45 degree
impact produces an oval
crater (Hoyt, 1987). Barringer, on the other hand, realized that a 45 degree
impact will produce a round
crater (Hoyt, 1987). Despite this insight, Barringer, like Gilbert,
initially assumed that the northern
Arizona impact had been vertical or nearly vertical and that the asteroid
was buried beneath the center of
the crater floor.

When extensive drilling did not locate a main mass beneath the crater floor
and instead only
produced traces of the projectile, Barringer began to consider other
options. He had already noted several
features that seem to have a directional symmetry.

- snip -

More recently, techniques similar to those of Sutton were applied by
Holliday et al. (2005) to the
Odessa impact site. They estimated the Odessa craters were produced
approximately 63,000 years ago.
Although the ages of Barringer and Odessa craters are still not precisely
known, these approximate ages
suggest Odessa formed earlier, with the caveat that the Barringer crater may
be older than 49,000 yrs.
(See discussion in Chapter 11). Thus, the two impact events may not be
directly related and may not have
any bearing on the issue of trajectory.

Nonetheless, several other potential indicators of trajectory survive (and
even the Odessa connection
might be revived). Unfortunately, these indicators cannot be reconciled at
the present time and I think it
fair to conclude that the trajectory of the impacting asteroid that produced
Barringer Crater remains
uncertain.

Chapter 9:
http://www.lpi.usra.edu/publications/books/barringer_crater_guidebook/chapte
r_9.pdf

Whole "guidebook":
http://www.lpi.usra.edu/publications/books/barringer_crater_guidebook/index.
shtml


Regards,

- John

Ontario, California


-Original Message-
From: meteorite-list-boun...@meteoritecentral.com
[mailto:meteorite-list-boun...@meteoritecentral.com] On Behalf Of
bernd.pa...@paulinet.de
Sent: Friday, September 10, 2010 3:26 AM
To: Meteorite-list@meteoritecentral.com
Subject: [meteorite-list] Meteor Crater Shape and Entry Angle

Eric wrote:

"The crater is not perfectly round as would be expected from an impactor 
coming in at a sharper angle. In fact the crater is more elliptical in
shape."

SHOEMAKER E.M. and KIEFFER S.W. (1974, 1979) Guidebook to the
Geology of Meteor Crater, Arizona (Publ. No. 17, Center for Meteorite
Studies, Arizona State University, Tempe, Arizona):

"Regional jointing has controlled the shape of the crater, which is somewhat
squarish in outline; the diagonals of the "square" coincide with the trend
of the
two main sets of joints. The largest tears occur in the "corners" of the
crater."

Eric also inquired:

"What would a "relatively low" impact angle be? 10 degrees, 20 degrees?"

I tried to find more precise information on that but was unable to find
something
that might be of help here. Maybe someone else can shed more light on this!

Regards,

Bernd

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[meteorite-list] Meteor Crater Shape and Entry Angle

2010-09-10 Thread bernd . pauli
Eric wrote:

"The crater is not perfectly round as would be expected from an impactor 
coming in at a sharper angle. In fact the crater is more elliptical in shape."

SHOEMAKER E.M. and KIEFFER S.W. (1974, 1979) Guidebook to the
Geology of Meteor Crater, Arizona (Publ. No. 17, Center for Meteorite
Studies, Arizona State University, Tempe, Arizona):

"Regional jointing has controlled the shape of the crater, which is somewhat
squarish in outline; the diagonals of the "square" coincide with the trend of 
the
two main sets of joints. The largest tears occur in the "corners" of the 
crater."

Eric also inquired:

"What would a "relatively low" impact angle be? 10 degrees, 20 degrees?"

I tried to find more precise information on that but was unable to find 
something
that might be of help here. Maybe someone else can shed more light on this!

Regards,

Bernd

__
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