Mars Exploration News  
On Mars No One Can Hear You Scream

These are not boils on Mars, but a way of depicting the surface magnetic fields on the planet to emphasize their ability to shield the surface from the solar wind. The greater the bulge, the stronger and more protective the magnetic field. Note that most of the remaining magnetic fields are in the southern hemisphere. Credit: David Brain/SSL
by Staff Writers
University Park PA (SPX) Jul 10, 2006
It may be difficult for two people to have a conversation on Mars, according to a research paper by Amanda Hanford and Lyle Long of the aerospace engineering department at Penn State University.

"Sound doesn't travel very far on Mars," explained Hanford, whose work is detailed in the paper, "Computer Simulations of the Propagation of Sound on Mars," which she recently presented at the 151st Acoustical Society of America meeting in Providence, R.I.

Using a Direct Simulation Monte Carlo method, Hanford and Long took into account the Martian atmospheric composition, as well as the lower atmospheric pressure of Mars and temperature differences.

"In studying sound on Mars, the physical properties of sound are the same," Hanford said, adding that Earth and Mars also share some physical similarities. The simulation predicted sound on Mars has a lower pitch and very short distance.

She said a sound's lower pitch is the result of the differences in the speed of sound. This is because of the red planet's atmospheric makeup - mostly carbon dioxide, with small percentages of nitrogen and argon with trace amounts of water vapor and oxygen.

"When you breathe in a helium balloon and speak, your voice is a high pitch," Hanford explained. "Assuming you could breathe in carbon dioxide (which is very toxic), your voice would be a lower pitch."

The distance sound can travel is also greatly affected by the Martian atmosphere.

"The lower pressure makes it so sound doesn't travel far," she said. According to the paper, sound generated by a human scream on Earth can travel a little over 1 kilometer (0.6 mile) before being absorbed completely by the atmosphere. On Mars, the sound from that same scream would only move about 16 yards at best.

Hanford created a downloadable movie clip of a DSMC-simulated sound wave propagating in the Martian atmosphere and its rate of decay.

The last attempt to record sound on Mars was part of the NASA's Mars Polar Lander, launched in January 1999. The probe included a miniature microphone to record sounds on the Martian surface. Communication with the lander was lost after it entered the Martian atmosphere on Dec. 3, 1999.

Community
Email This Article
Comment On This Article

Related Links
Acoustics Clip
Penn State
Mars News and Information at MarsDaily.com
Lunar Dreams and more



Memory Foam Mattress Review
Newsletters :: SpaceDaily :: SpaceWar :: TerraDaily :: Energy Daily
XML Feeds :: Space News :: Earth News :: War News :: Solar Energy News


Spirit Copes With Decreasing Solar Energy
Pasadena CA (SPX) Jul 07, 2006
With electrical power from Spirit's solar array down to about 300 watt-hours per Martian day, or sol, the science team is able to plan only one major activity per sol and often needs to devote one sol to recharging the rover's batteries.









  • Could NASA Get To Pluto Faster? Space Expert Says Yes - By Thinking Nuclear
  • NASA plans to send new robot to Jupiter
  • Los Alamos Hopes To Lead New Era Of Nuclear Space Tranportion With Jovian Mission
  • Boeing Selects Leader for Nuclear Space Systems Program

  • Pratt and Whitney Demonstrates Lunar Mission Propulsion System
  • SMART 1 Photographs Kepler Crater Up Close
  • Mysterious Lunar Swirls
  • SMART-1 Maneuvers Prepare For Mission End

  • Russian Soyuz Flights To Cost NASA 12 Million Dollars A Seat
  • South Korea Picking Astronauts
  • USA Partners With Pioneer Aerospace On CEV
  • Jules Verne ATV Passes Acoustic Tests

  • IAU Approves Names For Two Small Plutonian Moons
  • Three Trojan Asteroids Share Neptune Orbit
  • New Horizons Crosses The Asteroid Belt
  • Trio Of Neptunes And Their Belt

  • Gas Giants Consistently Larger Than Their Moons
  • Two Great Jovian Storms Converging
  • The Pull Of Jupiter
  • Hubble Takes Sharpest Shot Yet Of New Red Spot On Jupiter

  • Venus Express Spies Double Vortex
  • Venus Express Commissioning Phase Completed
  • Venus Express Reaches Final Mission Orbit
  • Venus Express Transmits First Images

  • Cassini Uncovering More Secrets Of Saturn Rings
  • Enceladus Exudes Air Of Mystery
  • Cassini Shines At Mission Halfway Point
  • NASA Makes Movies Of Saturn Moons In Motion

  • Research Office Helps Excite Oxygen to Make Laser
  • Falcon Supercomputer To Solve Problems
  • First Teraflop Class Supercomputer Decommissioned After 10 Years Service
  • AMPAC-ISP To Supply Loral With Thrusters For Telstar 11N Satellite

  • The content herein, unless otherwise known to be public domain, are Copyright 1995-2006 - SpaceDaily.AFP and UPI Wire Stories are copyright Agence France-Presse and United Press International. ESA PortalReports are copyright European Space Agency. All NASA sourced material is public domain. Additionalcopyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by SpaceDaily on any Web page published or hosted by SpaceDaily. Privacy Statement