[meteorite-list] Re: Scientists Find Mars Met. (NWA 1950)
From: MexicoDoug_at_aol.com <MexicoDoug_at_meteoritecentral.com>
Date: Thu Apr 22 10:31:57 2004 Message-ID: <174.2493e06b.2d29bd7b_at_aol.com> --part1_174.2493e06b.2d29bd7b_boundary Content-Type: text/plain; charset="UTF-8" Content-Transfer-Encoding: quoted-printable Content-Language: en I've alway had that exact same question: Where are the Earth meteorites? Th= e=20 answers I have contemplated are, which only plug the curiosity, and I=20 apologise if this is basic stuff published in some texts, as I have yet to r= ead and=20 meteorite reference materials except "Find a Falling Star": Tektites are a form of Earth Meteorites that didn't make escape velocity. =20 And we have plenty of them. >From a collision with the Earth, by an impacting stone or iron, anything=20 which DID obtain escape velocity from the Earth would do just that: escape.=20= It=20 would go any direction AWAY from the earth. The gravity of Earth is much greater than the minimal gravity of the=20 asteroids, and also greater than Mars or the Moon. So a much greater escape= velocity=20 is required to remove material from Earth. Additionally, Due to the atmosphere Earth has, at least atmospheric density=20 in the last X millions of years, a hot stone propelled from Earth would have= to=20 be fairly large to have it not dampened and returned to Earth. Thus, all=20 small stones would be quenched , by the atmosphere, medium stones exploded a= nd=20 quenched. That leaves very large stones... All the potential meteorites that have returned to Earth during the=20 provolking impact events timing have degraded and blended in with the surrou= nding rock,=20 except for some impact glasses, as glass as we all know is nearly=20 indestructable for millions of years. So it would have to be a rock returni= ng during the=20 last few dozen thousands of years. If Earth material is ejected in an orbit coincidentally similar to Earths, i= n=20 a few years the Earth will alter its course and sweep it up. Thus only very massive rocks sent AWAY from Earth's orbit would be potential= =20 meteorites. To actually become a meteorite on Earth, that big body would have to later=20 suffer a collision and be once again propelled towards Earth's orbit. The c= ase=20 with Mars is different since this material not swept out by Mars may settle=20 into near Earth's orbit over astronomical scales. Table: Escape velocity; Atmospheric density vs. Earth Earth 11.2 km/sec (25,000 mph); 1.00 Venus 10.4 km/sec (23,200 mph); 90 Mars 5.0 km/sec (11,200 mph); 0.01=20 Luna 2.4 km/sec (5,400 mph); 0.00 Vesta 0.39 km/sec (870 mph); none So you can see why there are no Venusian meteorites found yet -- ther=20 atmosphere is 90 times thicker than Earth's, similar gravity and escape velo= city (you=20 weigh 90% your Earth weight on Venus) and just as meteorites usually reach=20 free fall velocities when hitting Earth, to escape Earth, its the same in=20 reverse. One must ask, when was the last meteorite we know of that hit Eart= h at=20 more than free fall velocity? Perhaps Siberia (1908, the largest fall in th= e=20 last 2000 years, probably 400,000,000 Kg stone, known to have blown a man in= to a=20 tree forty feet away hundreds of km from impact, who later died of the injur= y)=20 ... no not even that one...it couldn't handle the atmosphere!!! So, the=20 small fragments upon an Earth impact typically would be blown to smitherines= =20 recaptured and fall immediately due to the atmospheric damping. And if they= are=20 Earth rocks, unless it is a fresh fall, one will never know as all but tekti= tes=20 disintegrate rapidly (less than a million years - excepting very special=20 preservation circumstances). If you look at my table atmospheres, you will see that the moon has none, an= d=20 Mars only 1% of Earth's. Add that to the fact that Escape velocity is less=20 than half for Mars, and for the Moon, almost down to a fifth, then mix in th= at=20 within 1,000,000 years, the Earth and Moon will sweep out virtually all of t= he=20 rocks that pass by its orbit, or change their orbit. In the case of Mars, the expulsion is more random from our point of view, an= d=20 although it is still unlikely, it is quite believable that some mass could b= e=20 orbiting, around, further modified by Jupiter and impacts in the asteroid=20 belt that can find its way to Earth. In the case of the Moon they should be= much=20 more common, except for the fact of the sweeping, they get cleaned out=20 quickly on an astronomic scale. If you still don't believe me, ask yourself (if you believe in Tektites):=20 What is the largest known tektite? That should make things clearer as to wh= at=20 happens to the resulting particles of a big impact, of the type necessary to= =20 make Earth meteorites, after the secondary shocking of atmospheric passage.=20= =20 Anyone have a one kilo tektite? And hot SiO2 I would guess is more cohesive= (=3D=20 larger fragments) than other "typical" Earth rocks. Those are the arguments I can come up with for the lack of Earth parented=20 meteorites. Of course, they are statistical, and a single rock doesn't foll= ow=20 statistics, just what happens to it...so don't give up looking for Earth=20 meteorites. PS I would expect the Moon to have conserved some Earth meteorites, and=20 perhaps some of the fresh Howardites contain ancient Earth meteorites. Saludos, Doug Dawn Mexico En un mensaje con fecha 01/04/2004 8:04:48 AM Mexico Standard Time,=20 cviau_at_beld.net escribe: >=20 > Really, can you imagine making an announcement like that and typo such=20 > important dating? >=20 > =20 >=20 > Your question is really a good one, and I have always thought that there=20 > MUST be some terrestrial =E2=80=98meteorites=E2=80=99 misclassified as bei= ng of=20 > extraterrestrial origin. >=20 > I also would like to hear a good reason why they are missing from the fin= d=20 > records. >=20 > =20 >=20 > Regards, >=20 > CharlyV >=20 > =20 >=20 > -----Original Message----- > From: meteorite-list-admin_at_meteoritecentral.com=20 > [mailto:meteorite-list-admin_at_meteoritecentral.com] On Behalf Of Fredmeteor= hall_at_aol.com > Sent: Sunday, January 04, 2004 4:29 AM > To: baalke_at_zagami.jpl.nasa.gov; meteorite-list@meteoritecentral.com > Subject: [meteorite-list] Re: Scientists Find Mars Met. (NWA 1950) >=20 > =20 >=20 > "SNC meteorites are extremely rare - fewer than 20 confirmed examples=20 > have been discovered - and are believed to all come from the same body of=20= rock.=20 > They are distinguished by their relative youth, being at most 1.3 million=20 > years old, compared to 4.5 million for other meteorites." From "Scientists= find=20 > Mars meteorite" "From Gerard Sevestre in Paris" January 04, 2004. > Hum, 1.3 million, 4.5 million? Not 1.3 billion and 4.5 billion? "fewer= =20 > than 20 confirmed examples"???=20 > Regards, Fred Hall > What was Earth's atmosphere like 1.3 Billion years ago? I'm sure Earth= =20 > had hydrated basaltic rocks then, right? Is there any possibility that som= e of=20 > the SNC's (lava meteorites) are not from Mars, but Earth? Isn't there an=20 > Earth meteor crater that formed around 1.3 billion years ago? I have yet=20= to=20 > hear a good reason as to why we have not found an "Earth meteorite". Some=20 > scientist out there, please set me straight as to why we have found some 2= 5+ Mars=20 > meteorites and not one Earth meteorite. > Thanks >=20 >=20 >=20 --part1_174.2493e06b.2d29bd7b_boundary Content-Type: text/html; charset="UTF-8" Content-Transfer-Encoding: quoted-printable Content-Language: en <HTML><FONT FACE=3Darial,helvetica><HTML><FONT SIZE=3D2 PTSIZE=3D10 FAMILY= =3D"SANSSERIF" FACE=3D"Arial" LANG=3D"0">I've alway had that exact same ques= tion: Where are the Earth meteorites? The answers I have contemplated=20= are, which only plug the curiosity, and I apologise if this is basic stuff p= ublished in some texts, as I have yet to read and meteorite reference materi= als except "Find a Falling Star":<BR> <BR> Tektites are a form of Earth Meteorites that didn't make escape velocity.&nb= sp; And we have plenty of them.<BR> <BR> >From a collision with the Earth, by an impacting stone or iron, anything whi= ch DID obtain escape velocity from the Earth would do just that: escape. It=20= would go any direction AWAY from the earth.<BR> <BR> The gravity of Earth is much greater than the minimal gravity of the asteroi= ds, and also greater than Mars or the Moon. So a much greater escape v= elocity is required to remove material from Earth.<BR> <BR> Additionally, Due to the atmosphere Earth has, at least atmospheric density=20= in the last X millions of years, a hot stone propelled from Earth would have= to be fairly large to have it not dampened and returned to Earth. Thu= s, all small stones would be quenched , by the atmosphere, medium stones exp= loded and quenched. That leaves very large stones...<BR> <BR> All the potential meteorites that have returned to Earth during the provolki= ng impact events timing have degraded and blended in with the surrounding ro= ck, except for some impact glasses, as glass as we all know is nearly indest= ructable for millions of years. So it would have to be a rock returnin= g during the last few dozen thousands of years.<BR> <BR> If Earth material is ejected in an orbit coincidentally similar to Earths, i= n a few years the Earth will alter its course and sweep it up.<BR> <BR> Thus only very massive rocks sent AWAY from Earth's orbit would be potential= meteorites.<BR> <BR> To actually become a meteorite on Earth, that big body would have to later s= uffer a collision and be once again propelled towards Earth's orbit. T= he case with Mars is different since this material not swept out by Mars may= settle into near Earth's orbit over astronomical scales.<BR> <BR> Table:<BR> Escape velocity; Atmospheric density vs. Earth<BR> <BR> Earth 11.2 km/sec (25,000 mph); 1.00<BR> Venus 10.4 km/sec (23,200 mph); 90<BR> Mars 5.0 km/sec (11,200 mph); 0.01 <BR> Luna 2.4 km/sec (5,400 mph); 0.00<BR> Vesta 0.39 km/sec (870 mph); none<BR> <BR> So you can see why there are no Venusian meteorites found yet -- ther atmosp= here is 90 times thicker than Earth's, similar gravity and escape velocity (= you weigh 90% your Earth weight on Venus) and just as meteorites usually rea= ch free fall velocities when hitting Earth, to escape Earth, its the same in= reverse. One must ask, when was the last meteorite we know of that hi= t Earth at more than free fall velocity? Perhaps Siberia (1908, the la= rgest fall in the last 2000 years, probably 400,000,000 Kg stone, known to h= ave blown a man into a tree forty feet away hundreds of km from impact, who=20= later died of the injury) ... no not even that one...it couldn't handle the=20= atmosphere!!! So, the small fragments upon an Earth impact typically w= ould be blown to smitherines recaptured and fall immediately due to the atmo= spheric damping. And if they are Earth rocks, unless it is a fresh fal= l, one will never know as all but tektites disintegrate rapidly (less than a= million years - excepting very special preservation circumstances).<BR> <BR> If you look at my table atmospheres, you will see that the moon has none, an= d Mars only 1% of Earth's. Add that to the fact that Escape velocity i= s less than half for Mars, and for the Moon, almost down to a fifth, then mi= x in that within 1,000,000 years, the Earth and Moon will sweep out virtuall= y all of the rocks that pass by its orbit, or change their orbit.<BR> <BR> In the case of Mars, the expulsion is more random from our point of view, an= d although it is still unlikely, it is quite believable that some mass could= be orbiting, around, further modified by Jupiter and impacts in the asteroi= d belt that can find its way to Earth. In the case of the Moon they sh= ould be much more common, except for the fact of the sweeping, they get clea= ned out quickly on an astronomic scale.<BR> <BR> If you still don't believe me, ask yourself (if you believe in Tektites): Wh= at is the largest known tektite? That should make things clearer as to= what happens to the resulting particles of a big impact, of the type necess= ary to make Earth meteorites, after the secondary shocking of atmospheric pa= ssage. Anyone have a one kilo tektite? And hot SiO2 I would gues= s is more cohesive (=3D larger fragments) than other "typical" Earth rocks.<= BR> <BR> Those are the arguments I can come up with for the lack of Earth parented me= teorites. Of course, they are statistical, and a single rock doesn't f= ollow statistics, just what happens to it...so don't give up looking for Ear= th meteorites.<BR> <BR> PS I would expect the Moon to have conserved some Earth meteorites, and perh= aps some of the fresh Howardites contain ancient Earth meteorites.<BR> <BR> Saludos,<BR> Doug Dawn<BR> Mexico<BR> <BR> <BR> En un mensaje con fecha 01/04/2004 8:04:48 AM Mexico Standard Time, cviau_at_be= ld.net escribe:<BR> <BR> <BLOCKQUOTE TYPE=3DCITE style=3D"BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT= : 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px"><BR> </FONT><FONT COLOR=3D"#000080" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:=20= #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG=3D"0"= >Really, can you imagine making an announcement like that and typo such impo= rtant dating?</FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKG= ROUND-COLOR: #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Aria= l" LANG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000080" BACK=3D"#ffffff" style=3D"BACKGROUND-C= OLOR: #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG= =3D"0"> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND= -COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LA= NG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000080" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:=20= #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG=3D"0"= >Your question is really a good one, and I have always thought that there MU= ST be some terrestrial =E2=80=98meteorites=E2=80=99 misclassified as being o= f extraterrestrial origin.</FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" s= tyle=3D"BACKGROUND-COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF"= FACE=3D"Arial" LANG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000080" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:= #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG=3D"0= ">I also would like to hear a good reason why they are missing from the find= records.</FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUN= D-COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" L= ANG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000080" BACK=3D"#ffffff" style=3D"BACKGROUND-C= OLOR: #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG= =3D"0"> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND= -COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LA= NG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000080" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:=20= #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG=3D"0"= >Regards,</FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUN= D-COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" L= ANG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:= #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SERIF" FACE=3D"Georgia" LANG=3D"0">= CharlyV</FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-= COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LAN= G=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000080" BACK=3D"#ffffff" style=3D"BACKGROUND-C= OLOR: #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG= =3D"0"> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND= -COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LA= NG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:=20= #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Tahoma" LANG=3D"0= ">-----Original Message-----<BR> <B>From:</B> meteorite-list-admin_at_meteoritecentral.com [mailto:meteorite-lis= t-admin_at_meteoritecentral.com] <B>On Behalf Of </B>Fredmeteorhall@aol.com<BR> <B>Sent:</B> Sunday, January 04, 2004 4:29 AM<BR> <B>To:</B> baalke_at_zagami.jpl.nasa.gov; meteorite-list@meteoritecentral.com<B= R> <B>Subject:</B> [meteorite-list] Re: Scientists Find Mars Met. (NWA 1950)</F= ONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR: #ff= ffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG=3D"0"><B= R> <BR> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-C= OLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SERIF" FACE=3D"Times New Roman= " LANG=3D"0"> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACK= GROUND-COLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Ari= al" LANG=3D"0"><BR> <BR> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:=20= #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SERIF" FACE=3D"Georgia" LANG=3D"0">&= nbsp; "SNC meteorites are extremely rare - fewer than 20 confirm= ed examples have been discovered - and are believed to all come from the sam= e body of rock. They are distinguished by their relative youth, being at mos= t 1.3 million years old, compared to 4.5 million for other meteorites." From= "Scientists find Mars meteorite" "From Gerard Sevestre in Paris" January 04= , 2004.<BR> Hum, 1.3 million, 4.5 million? Not 1.3 billion and 4.5 bi= llion? "fewer than 20 confirmed examples"??? <BR> Regards, Fred Hall<BR> What was Earth's atmosphere like 1.3 Billion years ago? I= 'm sure Earth had hydrated basaltic rocks then, right? Is there any possibil= ity that some of the SNC's (lava meteorites) are not from Mars, but Earth? I= sn't there an Earth meteor crater that formed around 1.3 billion years= ago? I have yet to hear a good reason as to why we have not found an "Earth= meteorite". Some scientist out there, please set me straight as to why we h= ave found some 25+ Mars meteorites and not one Earth meteorite.<BR> Thanks</FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-C= OLOR: #ffffff" SIZE=3D3 PTSIZE=3D12 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG= =3D"0"><BR> <BR> <BR> </BLOCKQUOTE><BR> </FONT><FONT COLOR=3D"#000000" BACK=3D"#ffffff" style=3D"BACKGROUND-COLOR:=20= #ffffff" SIZE=3D2 PTSIZE=3D10 FAMILY=3D"SANSSERIF" FACE=3D"Arial" LANG=3D"0"= ><BR> </FONT></HTML> --part1_174.2493e06b.2d29bd7b_boundary-- Received on Sun 04 Jan 2004 02:03:23 PM PST |
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