Planetary Profiles – Matt Wielicki
Planetary Insights – Impactites
Nov 17 2011: Mercury Revealed
Speakers
David Paige and Jean-Luc Margot
Dept. Earth & Space Sciences, UCLA
Abstract:
Profs. Paige and Margot will present new results from the MESSENGER
mission to Mercury, the first spacecraft to orbit the innermost
planet.
Planetary Profiles – Carolyn Crow
Cassini Chronicles Life of Saturn’s Giant Storm
New images and animated movies from NASA’s Cassini spacecraft chronicle the birth and evolution of the colossal storm that ravaged the northern face of Saturn for nearly a year.
These new full-color mosaics and animations show the storm from its emergence as a tiny spot in a single image almost one year ago, on Dec. 5, 2010, through its subsequent growth into a storm so large it completely encircled the planet by late January 2011.
The monster tempest, which extended north-south approximately 9,000 miles (15,000 kilometers), is the largest seen on Saturn in the past two decades and is the largest by far ever observed on the planet from an interplanetary spacecraft. On the same day that Cassini’s high-resolution cameras captured the first images of the storm, Cassini’s radio and plasma wave instrument detected the storm’s electrical activity, revealing it to be a convective thunderstorm. The storm’s active convecting phase ended in late June, but the turbulent clouds it created linger in the atmosphere today.
The storm’s 200-day active period also makes it the longest-lasting planet-encircling storm ever seen on Saturn. The previous record holder was an outburst sighted in 1903, which lingered for 150 days. The large disturbance imaged 21 years ago by NASA’s Hubble Space Telescope and comparable in size to the current storm lasted for only 55 days.
Planetary Insights – Plasma Waves
Planetary Profiles – Mike Hartinger
Interview with UCLA’s Michael Hartinger
Nov 10 2011: Solar Variability and the Sun-Earth Connection
Speaker:
Dr. Karel Schrijver
Lockheed-Martin Advanced Technology Center
Abstract:
The Sun’s evolving magnetic field causes variations in solar
irradiance, heliospheric wind, and geospace conditions that range from
seconds-long explosions to billion-year trends. Traces of that
variability can be found in Galileo’s drawings and ancient ice sheets,
while observations of stars like the Sun provide glimpses of what the
Sun did through the ages. This observational material guides us towards
an understanding of the root of solar activity – the dynamo – needed to
understand the Sun-Earth connections.