HONOLULU — Curiosity, the NASA rover that landed on Mars last month, is sending remarkable weather observations from the Martian surface that are attracting interest from scientists, the University of Hawai‘i reported Monday. “From a weather point of view, Mars
HONOLULU — Curiosity, the NASA rover that landed on Mars last month, is sending remarkable weather observations from the Martian surface that are attracting interest from scientists, the University of Hawai‘i reported Monday.
“From a weather point of view, Mars is the most ‘Earth-like’ of the other planets in our solar system, and many features of the weather there are similar to Earth,” said Kevin Hamilton, a pioneer in the area of computer modeling of the Martian atmosphere.
Hamilton, the Director of UH Manoa’s International Pacific Research Center and a meteorology professor, noted that Curiosity is the fifth “Weather Station” on Mars. Over the last 35 years, a total of four NASA probes had reached the Martian surface and returned weather data.
“These earlier observations had shown a large daily cycle in temperature and air pressure on Mars. The atmospheric temperature near the surface of Mars generally varies by more than 100 degrees Fahrenheit between day and night because of the overall thinner Martian atmosphere and lack of oceans and their moderating influence,” Hamilton said.
“The exciting new result from Curiosity is a regular and truly enormous swing in atmospheric pressure through each day. Measurements on Earth show a daily swing in pressure of only about one-tenth of 1 percent of the mean pressure, whereas Curiosity is measuring swings of almost 10 percent of the daily average pressure. We observe such a relative pressure change on Earth only with the passage of an extremely strong hurricane. At the Curiosity site on Mars, this enormous pressure swing occurs regularly every day.”
For Hamilton, these reports of huge pressure swings came as welcome news. Almost 20 years ago, he had predicted that the daily variation on Mars would be particularly large in two “action centers” on the equator located on opposite sides of the Mars. Unlike the earlier NASA probes, Curiosity landed right in one of the equatorial action centers, where another factor comes into play: a resonance in the Martian atmosphere.
“The idea of resonance is familiar in everyday contexts like pushing a child in a playground swing — if you synchronize your pushes with the natural frequency of the swing, it is easy to send the child high into the air,” Hamilton said.
“In the 1980s, I calculated that on Mars the atmosphere could have a natural frequency with the period of one Martian day. The day-night forcing then could excite a very strong resonant response. Incorporating this idea into a sophisticated computer model, I showed that the effect of this resonant response would be most clearly felt in two equatorial action centers and that the pressure swings there should exceed 8 percent of the mean pressure. The remarkable Curiosity observations provide strong confirmation of a resonant vibration of the global atmosphere.”
Hamilton suggests that the daily resonant cycles could play a role in explaining a long-standing mystery on Mars, namely how the winds become sufficiently strong to lift enough dust from the surface to create the remarkable global dust storms seen every few years on that planet.
“Now that my theory of a daily resonant oscillation seems confirmed, it might help explain the trigger for these dust storms,” he said.