Twin ARTEMIS probes to study Moon in 3-D
The mission will involve observations of the lunar surface, its magnetic field, and the surrounding magnetic environment.
July 15, 2011
On Sunday, July 17, the Moon will acquire its second new companion in less than a month. That’s when the second of two probes built by the University of California, Berkeley, and part of NASA’s five-satellite Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission will drop into a permanent lunar orbit after a meandering 2-year journey from its original orbit around Earth.
Pictorial representation of the ARTEMIS probes as they will orbit the moon beginning July 17. ARTEMIS P1 and P2 were the outermost two THEMIS probes before they began maneuvers July 20, 2009, to swap an Earth orbit for a lunar orbit. Credit: UC Berkeley
The first of the two probes settled into a stable orbit around the Moon’s equator June 27. If all goes well, the second probe will assume a similar lunar orbit, though in the opposite direction, sometime Sunday afternoon. The two spacecraft that constitute the Acceleration, Reconnection, Turbulence, and Electrodynamics of the Moon’s Interaction with the Sun (ARTEMIS) mission will immediately begin the first observations ever conducted by a pair of satellites of the lunar surface, its magnetic field, and the surrounding magnetic environment.
“With two spacecraft orbiting in opposite directions, we can acquire a full 3-D view of the structure of the magnetic fields near the Moon and on the lunar surface,” said Vassilis Angelopoulos from the University of California, Los Angeles. “ARTEMIS will be doing totally new science, as well as reusing existing spacecraft to save a lot of taxpayer money.”
“These are the most fully equipped spacecraft that have ever gone to the Moon,” added David Sibeck from NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “For the first time, we’re getting a unique, two-point perspective of the Moon from two spacecraft, and that will be a major component of our overall lunar research program.”
The transition into a lunar orbit will be handled by engineers at the University of California’s Berkeley’s Space Sciences Laboratory (SSL), which serves as mission control both for THEMIS and ARTEMIS.
What Makes the Aurorae Dance?
NASA launched the five THEMIS satellites February 17, 2007, to explore how the Sun’s magnetic field and million-mile-per-hour solar wind interact with Earth’s magnetic field on Earth’s leeward side, opposite the Sun. Within a year and a half, they had answered the mission’s primary question: Where and how do substorms in the Earth’s magnetosphere — which make the aurorae at the North and South Poles dance — originate?
The answer: the storms originate deep in the planet’s shadow, about a third of the way to the Moon, where magnetic field lines snap, reconnect, and unleash a storm of energy that funnels to the poles and makes the atmosphere glow in reds and greens. Large storms can wreak havoc on satellites, power grids, and communications systems.
Mission accomplished, the THEMIS team was eager to divert two of the probes to the Moon to extend their magnetic field studies farther into space. One key reason was that the two probes most distant from Earth would soon die because, with too much time spent in Earth’s shadow, their solar-powered batteries would discharge.
To achieve this new mission, the UC Berkeley and Goddard teams, with the assistance of experts at NASA’s Jet Propulsion Laboratory in Pasadena, California, charted the 150 fuel-saving orbital maneuvers needed to boost the two THEMIS spacecraft from Earth’s orbit into temporary orbits around the two Earth-Moon Lagrange points, which are spots in space where the gravitational attraction from the Moon and Earth are equal. That transfer took about 18 months, after which Goddard colleagues kept the two spacecraft in Lagrange-point orbits for several months before the first probe (P1) was transferred into lunar orbit last month.
“That was an engineering challenge; this is the first mission where we’ve piloted into a lunar orbit spacecraft not designed to go there,” said Daniel Cosgrove from UC Berkeley. The probes’ small thrusters, for example, only push down and sideways. The probes are also spinning, which makes maneuvering even more difficult.
Also, last year probe P1 lost a spherical sensor from the end of one of four long wires that protrude from the spacecraft to measure electrical fields in space. The probable cause was a micrometeorite that cut a 10-foot (3 meters) section off of the 82-foot (25m) wire and caused it to retract into its original spherical housing, sending the “little black sphere flying through the solar system,” Bester said.
Side view of the ARTEMIS P1 probe's orbit in 2010 as it cruised around the two Earth-moon Lagrange points. In 2011, it maneuvered into a permanent orbit around the Moon. Credit: NASA
“All five spacecraft have been built by a very talented team with enormous attention to detail,” he said, predicting that the ARTEMIS probes could survive for another 10 years, longer than the three remaining THEMIS probes, which repeatedly fly in and out of Earth’s dangerous Van Allen radiation belt.
Once the second probe (P2) is in orbit, the two ARTEMIS satellites will graze the lunar surface once per orbit — approaching within a few tens of miles — in a belt ranging 20° above and below the equator while recording electric and magnetic fields and ion concentrations.
“When the Moon traverses the solar wind, the magnetic field embedded in the rocks near the surface interacts with the solar wind magnetic field, while the surface itself absorbs the solar wind particles, creating a cavity behind the Moon,” Angelopoulos said. “We can study these complex interactions to learn much about the Moon as well as the solar wind itself from a unique two-point vantage that reveals for the first time 3-D structures and dynamics.”
Sibeck noted that NASA’s twin STEREO spacecraft, launched in 2006, already provide a 3-D perspective on the Sun’s large-scale magnetic fields. “THEMIS and ARTEMIS study the microscale processes, which we now know run the system,” he said.
One goal of the ARTEMIS mission is to look for plasmoids, which are hot blobs of ionized gas or plasma.
“THEMIS found evidence that magnetic reconnection propels hot blobs of plasma both towards and away from the Earth, and we want to find out how big they are and how much energy they carry,” Angelopoulos said. “Plasmoids could be tens of thousands of miles across.”
“THEMIS found the cause and now ARTEMIS will study the consequences, which are likely massive and global,” Sibeck said.
The spacecraft also will study the surface composition of the Moon by recording the solar wind particles reflected or scattered from the surface and the ions sputtered out of the surface by the wind.
“These measurements can tell us about the properties of the surface, from which we can infer the formation and evolution of the surface over billions of years,” Angelopoulos said.
The two ARTEMIS probes will join NASA’s Lunar Reconnaissance Orbiter, which has been orbiting the Moon since 2009 and taking high-resolution photographs and looking for signs of water ice. In September, NASA is scheduled to launch two Gravity Recovery and Interior Laboratory (GRAIL) spacecraft to map the Moon’s gravitational field, and in 2013, the agency plans to launch the Lunar Atmosphere and Dust Environment Explorer (LADEE) to characterize the lunar atmosphere and dust environment.
“ARTEMIS will provide context for the LADEE mission,” Sibeck said.
Three other non-functioning satellites remain in orbit around the Moon: two sub-satellites of Japan’s lunar orbiter, Kaguya, which was guided to a crash on the surface in 2009; and India’s Chandrayaan-1, which lost communication with Earth that same year. China’s second lunar orbiter, Chang’e 2, left the Moon for interplanetary space June 8.
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