[meteorite-list] Martian Meteorite Heat Ablation?
From: Sterling K. Webb <sterling_k_webb_at_meteoritecentral.com>
Date: Wed, 8 Aug 2007 15:41:22 -0500 Message-ID: <013b01c7d9fc$7bf97340$ac2ee146_at_ATARIENGINE> Hi, Chris, and List, > Presumably, meteors begin burning somewhat > lower on Mars, and have a greater chance of reaching > the surface... The rate at which pressure declines with altitude is characterized by the scale height, the altitude at which pressure has dropped by a factor of "e" (nat. log. base = 2.72forever). The scale height of the Martian atmosphere is about 11 kilometers; for the Earth it's only about 6 kilometers. The formula for the scale height is H = ( k * T ) / ( M * g ), where k = Gas constant = 8.314 J?(mole K)^-1, T = mean planetary surface temperature in kelvin degrees, M = mean molecular mass of dry air (units kg?molec ^-1), g = acceleration due to gravity on planetary surface. Molecular mass of the Martian atmosphere is about 50% greater then the Earth's "M," but "g" is 38% of the Earth's. Planets with lower gravity have "taller" atmospheres, if you want to remember it the easy way. There are always "wrinkles" to ideal gas formulas. At very high altitudes, the "air" is so thin that diffusion is easy, so every species of gas molecule has "its own" scale height. But Mars is mostly carbon dioxide, so that doesn't change things much. Atmospheric pressure on the surface of Mars varies from around 30 Pascals on Olympus Mons to over 1155 Pascals in the depths of Hellas Planitia, with a mean surface level pressure of 600 Pascals. This is less than 1% of the surface pressure on Earth (101,300 Pascals). The equivalent pressure in the atmospheres of the two planets can be found in Mars' thin atmosphere at a height of 35 km above either planet's surface. Another implication for the case of a meteorite entry is that the Martian atmosphere at 60 to 80 kilometers above the surface is DENSER than the atmosphere of the Earth at that height. All Martian densities at altitudes above 34 kilometers are, due to the fact that the pressure (hence density, since the pressure of a planetary atmosphere is a function of its mass) falls off less steeply than is the case in the Earth's atmosphere. So, the meteoroid that "lights up" at 60 km in the Earth's atmosphere, will presumably "light up" at a higher altitude in the Martian atmosphere. It may very well terminate its ablative flight at a higher altitude (if that happens above 34 kilometers) or a lower altitude (if that happens above 34 kilometers) than it would in the Earth's atmosphere, and have a correspondingly longer or shorter "dark fall" (but a much slower fall due to the lesser Martian gravity). Ouch! It's hard to think outside your own gravity well! Now, I'm going to hand the calculator back to Chris... Sterling K. Webb ------------------------------------------------------------------------------ ----- Original Message ----- From: "Chris Peterson" <clp at alumni.caltech.edu> To: "Meteorite List" <meteorite-list at meteoritecentral.com> Sent: Wednesday, August 08, 2007 12:21 PM Subject: Re: [meteorite-list] Martian Meteorite Heat Ablation? But Mars does have an atmosphere. Its surface air density is about the same as Earth's at a height of 31 km, and far more than the density in the region of Earth's atmosphere where we typically see meteors. Presumably, meteors begin burning somewhat lower on Mars, and have a greater chance of reaching the surface. But meteoroids certainly ablate as they pass through the Martian atmosphere. On Mars, it really is likely that a meteorite might be hot when it lands! BTW, meteors have been recorded by cameras on Mars. Chris ***************************************** Chris L Peterson Cloudbait Observatory http://www.cloudbait.com ----- Original Message ----- From: "Mike Groetz" <mpg444 at yahoo.com> To: "Meteorite List" <meteorite-list at meteoritecentral.com> Sent: Wednesday, August 08, 2007 10:59 AM Subject: [meteorite-list] Martian Meteorite Heat Ablation? > Hi Everyone- > Assuming Mars does not have an atmosphere and the > pitting in this rover photo of a meteorite on Mars is > from heat ablation... > > http://www.space.com/php/multimedia/imagedisplay/img_display.php?pic=h_opportunity_rock0120_1_02.jpg&cap=Instruments+on+the+Opportunity+Mars+rover+were+used+to+determine+that+the+object+was+a+meteorite.+Image+Credit%3A+NASA%2FJPL > > Would this be possible without an atmosphere? > Take care, stay cool. > Thank you > Mike Received on Wed 08 Aug 2007 04:41:22 PM PDT |
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