
Perseid meteor Astrophotographer Jeff Berkes caught this Perseid meteor over the Hawaiian island of Kauai in 2010.
Image: Jeff Berkes
Meteoroids streaking through the atmospheres of planets such as Earth, Mars and Venus can change these worlds' air, in ways that researchers are just now beginning to understand.
Most planetary atmospheres are made up of simple, low-mass elements and compounds such as carbon dioxide, oxygen and nitrogen. But when a debris particle, or meteoroid, passes through, it can shed heavier, more exotic elements such as magnesium, silicon and iron.
Such elements can have a significant impact on the circulation and dynamics of winds in the atmosphere, researchers say.
"That opens up a whole new network of chemical pathways not usually there," said Paul Withers of Boston University. [Infographic: Earth's Atmosphere Top to Bottom]
Contaminating the outer layers
Part of a planet's upper atmosphere, the ionosphere contains plasma — a mixture of positively charged (ionized) atoms or molecules and the negatively charged electrons stripped from them. When simple elements such as oxygen move into this outer shell, they break apart easily, decaying in a matter of minutes.
But meteoroids streaking toward a planet's surface carry heavier metals that can be removed in a variety of ways. A grain of dust, for instance, may rapidly burn up, shedding already-ionized magnesium as it falls. Or, neutral magnesium may be torn from the small rock, then receive a charge from sunlight or from stripping an electron from another particle. The newly charged elements can take as much as a full day to decay.
Meteoroids that blaze a trail through the atmosphere are called meteors, or shooting stars. Only those that make it to the ground are meteorites.
"When we add metal ions to the ionosphere as a result of this meteoroid input, we create plasma in regions where there wasn't any plasma there to start out with," Withers told SPACE.com.
In a recent article for Eos, the American Geophysical Union's newspaper covering Earth and space sciences, Withers discusses important questions raised by the recent wealth of research on the upper atmosphere of Mars and Venus.
Shocking similarities, strange differences
Over the last decade, scientists have collected more and more information about the ionospheres of Mars and Venus. Though one might envision the composition and location of the two planets would create different interactions in the ionosphere, the two are actually very similar, scientists say. [Video: Does the Moon Have a Strange Ionosphere?]
"If you stand at the surface of the two planets, they are very different," Withers said. "But up at about 100 kilometers (62 miles), conditions are surprisingly similar."
The pressures, temperatures, and chemistry at high altitudes are comparable for the two planets. So too are many of the properties of the layers of charged particles shed by meteoroids.
"The plasma densities are quite similar on average on all three planets, which is not what you might expect on the first impression," Withers said, referring to Earth, Mars and Venus.
Since the sun is the ultimate driving force for most ionization processes, it's tempting to assume that Venus has more particles in a given area than Mars does because it orbits twice as closely to our star. Instead, the two planets have similar densities, which differ from Earth's measurements by only a factor of ten.



See what we're tweeting about




2 Comments
Add CommentThe article at one stage states :
Reply | Report Abuse | Link to this"Since the sun is the ultimate driving force for most ionization processes, it's tempting to assume that Venus has more particles in a given area than Mars does because it orbits twice as closely to our star. Instead, the two planets have similar densities, which differ from Earth's measurements by only a factor of ten."
Density of ionization is a function of the distance from Sun. But article states that Mars and Venus have same densities though separated from Sun far part. Then density of ionization in ionosphere of earth differ from Mars or Venus by a factor of 10. More or less? Article does nos provides clarity. Further article also does not furnishes any clarity on the observed anomaly of density of ionization in Venus, Earth and Mars
I second the points raised by vinodkumarsehgal. A factor of 10 isn't negligible.
Reply | Report Abuse | Link to this