Google+ SpaceTravelFoundation: Aurora
Showing posts with label Aurora. Show all posts
Showing posts with label Aurora. Show all posts

February 18, 2015

Mystery haze found on Mars surprises scientists

Dear readers and followers,

Enormous cloud-like plumes reaching 260 kilometers above the surface of Mars have left scientists baffled. This is way beyond Mars’ normal weather, reaching into the exosphere where the atmosphere merges with interplanetary space. None of the conventional explanations for such clouds make sense, neither water or carbon dioxide ice nor dust storms nor auroral light emissions usually hit such heights.



These “mystery clouds” came as a surprise, in particular when considering they were first spotted by a string of amateur astronomers in 2012. After all, an international fleet of five orbiters and two rovers is currently operating on and around Mars, and one may be excused thinking the red planet has little left to hide and its exploration has become routine.

A survey of images from the +Hubble Space Telescope and amateur astronomers revealed massive clouds had been seen on Mars before, but none as prominent as the 2012 observations.

Perhaps these clouds could be aurorae, similar to the northern lights (aurora borealis) here on Earth, or their southern counterpart aurora australis. These displays happen when the Earth’s magnetic field channels charged particles emitted by the Sun towards the poles, where they interact with the atmosphere and emit light.

Mars does not have a global magnetic field, only pockets of magnetization. The mystery clouds were spotted over one of these so-called magnetic anomalies, and auroral lights have been observed there previously.

However, to explain the 2012 observations, an aurora would have had to be 1,000 times brighter than the northern lights. This would require an increased flow of charged particles from the sun, but its activity was not unusually high during the time. Could dust be the culprit? A volcanic eruption or an asteroid impact were among the earliest theories about these clouds’ origin. New eruptions on Mars are plausible, though we’re yet to observe any active volcanoes on the planet. The youngest lava flows reported are a few million to tens of million years old, which is recent in geological terms.



Mars’ thin atmosphere offers little protection against asteroids, and its surface is pockmarked with impact craters. Cameras on board NASA’s Mars Reconnaissance Orbiter have documented the appearance of hundreds of new craters in the nine years since the spacecraft arrived at Mars.

However, both theories were quickly discarded because they were inconsistent with the behavior of the clouds. Continued observations showed that they disappeared during the Martian daytime, were not visible in the evening, and reappeared each morning for at least ten consecutive days.

This also rules out dust storms, which frequently engulf large areas of the planet’s surface. Furthermore, the wavelength profile of the light reflected by the mystery clouds is a poor match for Martian dust particles. That leaves water or carbon dioxide ice particles, which fit the wavelength profile of the reflected light. Both water and carbon dioxide molecules also occur naturally in the atmosphere at these heights.

However, to form these clouds both substances would need to condense into ice particles. This would require the atmospheric temperature at these heights to drop suddenly by up to 100˚C. We’ve no idea what would cause such a drop, and we’re yet to spot such a massive, localized cold snap.

Sánchez-Lavega and colleagues thus declare that their “explanations defy our current understanding of Mars’ upper atmosphere” and their investigation only partially lifts the shroud surrounding these mysterious clouds.

High altitude clouds are not the only Martian mysteries keeping researchers on their toes. One question driving the exploration of the red planet is whether there has ever been life on Mars. Latest results by NASA’s Curiosity rover reaffirm that the planet provided habitable conditions in its past.

Water is the most important prerequisite for life. One explanation for the ongoing formation of gullies and related features, for example, is liquid water at or near the Martian surface even during the currently prevailing extreme dry and cold conditions. And while there are many possible explanations for the enigmatic whiffs of methane observed on Mars, one of the most exciting is the production by microorganisms living just below the surface.

Part of the fascination of Mars exploration is that it is very much about understanding our own origins and future. As the example of the mystery cloud observations shows, everybody has a chance to participate in unraveling the red planet’s mysteries.

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February 5, 2015

NASA launched a rocket into Northern Lights

Dear readers and followers,


The interaction of the solar wind (issue from the Sun ) and Earth’s atmosphere produces auroras. These northern and southern lights dance across the night sky and have mesmerized and inspired observers for centuries. For scientists, this dance of light also leads to many questions about how space weather affects Earth’s atmosphere. In late January 2015, scientists, in collaboration with NASA, launched a rocket with probes into the northern lights in order to learn more about how they heat the planet’s atmosphere.  

Credit image: +NASA 

The Auroral Spatial Structures Probe (ASSP) was launched at 5:41 a.m. on January 28th 2015, from the Poker Flat Research Range about 50 kilometers north of Fairbanks, Alaska. 

The ASSP carried seven instruments to study the electromagnetic energy that can heat the thermosphere, the second highest layer of the atmosphere, during auroral events. The interaction of waves and particles from the solar wind, Earth’s magnetosphere, and the upper atmosphere can cause “Joule heating.” Essentially, the electrical currents on the edge of space run into a resistant media (the air in the atmosphere) and generate heat in a process similar to that of a toaster coil or electric stove. This heating can expand the atmosphere upward and increase the friction, or drag, on spacecraft and satellites.

The AASP launch occurred just two days after the successful launches of the Mesosphere-Lower Thermosphere Turbulence Experiment (M-TeX) and the Mesospheric Inversion-layer Stratified Turbulence (MIST) experiment. Two pairs of instrumented rockets were launched about 30 minutes apart to study how turbulence is formed in the presence of inversion layers in the upper atmosphere. This turbulence causes particles to diffuse between atmospheric layers. The MIST launches included the release of harmless trimethyl aluminum vapor to help researchers trace diffusion at high altitude

“Recent solar storms have resulted in major changes to the composition of the upper atmosphere above 80 kilometers, where enhancements in nitrogen compounds have been found,” said Richard Collins, upper atmospheric researcher from the University of Alaska. “These compounds can be transported into the middle atmosphere where they can contribute to ozone destruction. However, the meteorological conditions do not always allow such transport to occur. Thus, the impact of solar activity on the Earth is not just about how the Sun is a source of energetic particles, but also how the Earth’s meteorological conditions determine the fate of these particles in the atmosphere.”



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