Out of THEMIS, ARTEMIS: Earth's loss is moon's gain

Oct 27, 2010 By Robert Sanders
An artist's concept of one of the twin ARTEMIS probes in orbit around the moon. Formerly part of the THEMIS suite of five probes in Earth orbit, these two micro-satellites will now observe the solar wind's impact on the Earth's magnetic field at a much greater distance from Earth, and the wake left by the moon as it travels through the magnetosphere. Credit: NASA Goddard Space Flight Center

(PhysOrg.com) -- Two micro-satellites originally launched into Earth's orbit in 2007 by NASA have been redirected by University of California, Berkeley, scientists toward new orbits around the moon, extending study of the earth and moon's interaction with the solar wind.

The second of the two probes settled into a temporary "Lagrange-point" orbit on Friday, Oct. 22, inaugurating science operations for a new mission dubbed ARTEMIS – Acceleration, Reconnection, Turbulence, and Electrodynamics of the Moon's Interaction with the Sun.

Lagrange points are places where the gravity of Earth and the balance, creating a sort of gravitational parking lot for spacecraft. The two probes will remain there for six months before transitioning to their final, lunar orbits.

Over the next several years, ARTEMIS will help space scientists understand how the earth's magnetosphere is shaped by the strong solar wind at the distance of the moon and also how the moon's own tiny magnetic field interacts with the solar wind. Using simultaneous measurements of particles and electric and magnetic fields from two locations, ARTEMIS will provide the first three-dimensional perspective of how energetic particle acceleration occurs near the moon's orbit, in the distant magnetosphere, and in the solar wind.

"We currently know very little regarding the space environment of the moon, despite a number of existing and planned observatories there," said Vassilis Angelopoulos, principle investigator for the ARTEMIS mission and a professor of space physics at UCLA. "ARTEMIS is on stable orbits and can provide valuable information regarding the space environment, especially during the approaching solar maximum, as well as fully explore the earth's environment at lunar distances for the first time."

The two probes were originally part of NASA's five-probe THEMIS (Time History of Events and Macroscale Interactions during Substorms) mission, built and operated by UC Berkeley to orbit Earth and determine how storms in the earth's magnetic field disturb the colorful auroras in the Northern and Southern hemispheres.

THEMIS completed is primary mission in 2008 when Angelopoulos announced, "We discovered what makes the Northern Lights dance." The THEMIS team then proposed that the two outermost of the five probes use their extra fuel to propel themselves, via complex maneuvers around the moon and Earth, into lunar orbits – the first two-satellite mission to the moon. The maneuvers would also save the solar-powered spacecraft, which were spending more and more time in the earth's shadow and, for lack of power, in danger of freezing to death.

The two ARTEMIS probes will orbit for about six months around the Lagrange points near the moon before descending to final orbits around the moon. The Lagrange points are places where the gravity of the Earth and moon cancel one another, creating a sort of parking lot for satellites or debris. (Image: NASA Goddard Space Flight Center)

After approval from , Angelopoulos and his UC Berkeley team, which operates the fleet of satellites from the campus's Space Sciences Laboratory (SSL), began to reposition the two probes on July 20, 2009. The first probe (P1) settled into an orbit around the L2 Lagrange point, located on the far side of the moon, on Aug. 25, 2010, and is now joined by the second (P2) in orbit around the L1 Lagrange point between Earth and moon.

"ARTEMIS is going where no spacecraft have gone before," said Manfred Bester, director of operations at SSL. "We are exploring the Earth-moon Lagrange points for the first time."

Because the Lagrange points lie just outside Earth's magnetosphere, they are excellent places from which to study the solar wind. Particle and field sensors onboard the ARTEMIS probes have access to solar wind streams and storm clouds as they approach Earth, a possible boon to space weather forecasters. Moreover, working from opposite Lagrange points, the two spacecraft will be able to measure solar wind turbulence on scales never sampled by previous missions.

"ARTEMIS is going to give us a fundamental new understanding of the solar wind," predicted David Sibeck, ARTEMIS project scientist at the Goddard Space Flight Center in Maryland.

ARTEMIS will also explore the moon's plasma wake – a turbulent cavity carved out of the solar wind by the moon itself, akin to the wake just behind a speedboat. Sibeck called this "a giant natural laboratory filled with a whole zoo of plasma waves waiting to be discovered and studied."

Plasmas are hot, ionized clouds of gas that can carry electromagnetic and electrostatic waves.

Another target of the ARTEMIS mission is Earth's magnetotail. Like a wind sock at an airport, Earth's magnetic field is elongated by the action of the solar wind, forming a tail that stretches to the orbit of the moon and beyond. Once a month around the time of the full moon, the ARTEMIS probes will follow the moon through the magnetotail.

"We are particularly hoping to catch some magnetic reconnection events," says Sibeck. "These are explosions in Earth's magnetotail that mimic solar flares, albeit on a much smaller scale."

ARTEMIS might even see giant 'plasmoids' accelerated by the explosions hitting the moon during magnetic storms. Plasmoids are self-contained balls of plasma and magnetic field that can carom off reconfiguring planetary magnetic fields in space like billiard balls.

These far-out explorations may have down-to-Earth applications, Angelopoulos said. Plasma waves and reconnection events pop up on Earth, such as in experimental fusion chambers. Fundamental discoveries by ARTEMIS could help advance research in the area of clean renewable energy.

After six months at the Lagrange points, ARTEMIS will move in closer to the moon, at first only 100 kilometers from the surface, but eventually even closer. From point-blank range, the spacecraft will look to see what the solar wind does to a rocky world when there is no magnetic field to protect it.

"Earth is protected from solar wind by the planetary ," explained Angelopoulos. "The moon, on the other hand, is utterly exposed. It has no global magnetism."

Studying how the electrifies, alters and erodes the moon's surface could reveal valuable information for future explorers and give planetary scientists a hint of what's happening on other unmagnetized worlds around the solar system.

Orbiting the moon is notoriously tricky because of irregularities in the lunar gravitational field. Enormous concentrations of mass – mascons – hide just below the surface and tug on spacecraft in unexpected ways, causing them over time to veer out of orbit, Angelopoulos said. ARTEMIS will mitigate this problem using highly elongated orbits, ranging from tens of kilometers to 18,000 kilometers.

"We'll zip by the lunar surface for a brief time each orbit," explained Angelopoulos. "Most of the time we'll linger 18,000 kilometers away where we can continue our studies of the at a safe distance. But over several years, even the sparse low-altitude measurements add up to a sizeable dataset."

ARTEMIS will work in tandem with current missions, such as NASA's Lunar Reconnaissance Orbiter, LADEE (Lunar Atmosphere and Dust Environment Explorer) and Grail (Gravity Recovery and Interior Laboratory), and Chang'e 2, a Chinese unmanned probe, to prepare the ground for increased robotic exploration of the moon by future U.S. missions, including the international lunar network.

Explore further: We are all made of stars

Provided by University of California -- Berkeley

4.7 /5 (7 votes)

Related Stories

ARTEMIS - the first Earth-Moon libration orbiter

Sep 14, 2010

In August 1960, NASA launched its first communications satellite, Echo 1. Fifty years later, NASA has achieved another first by placing the ARTEMIS-P1 spacecraft into a unique orbit behind the moon, but not ...

ARTEMIS spacecraft believed stuck by object

Oct 25, 2010

Flight Dynamics data from THEMIS-B (one of the two ARTEMIS spacecraft) indicated that one of the EFI (electric field instrument)spherical tip masses may have been struck by a meteoroid at 0605 UT on October ...

Satellites Will Improve Understanding of the Sun

Aug 17, 2006

NASA's Solar Terrestrial Relations Observatory mission will dramatically improve understanding of the powerful solar eruptions that can send more than a billion tons of the sun's outer atmosphere hurtling into ...

Magnetic anomalies shield the Moon

Sep 28, 2010

Scientists have discovered a new type of solar wind interaction with airless bodies in our solar system. Magnetized regions called magnetic anomalies, mostly on the far side of the Moon, were found to strongly ...

NASA Satellites Discover What Powers Northern Lights

Jul 24, 2008

(PhysOrg.com) -- Researchers using a fleet of five NASA satellites have discovered that explosions of magnetic energy a third of the way to the moon power substorms that cause sudden brightenings and rapid movements of the ...

Recommended for you

Observing the onset of a magnetic substorm

15 hours ago

Magnetic substorms, the disruptions in geomagnetic activity that cause brightening of aurora, may sometimes be driven by a different process than generally thought, a new study in the Journal of Geophysical Research: Space Ph ...

We are all made of stars

17 hours ago

Astronomers spend most of their time contemplating the universe, quite comfortable in the knowledge that we are just a speck among billions of planets, stars and galaxies. But last week, the Australian astronomical ...

ESA video: The ATV-5 Georges Lemaitre loading process

17 hours ago

This time-lapse video shows the ATV-5 Georges Lemaitre loading process and its integration on the Ariane 5 launcher before its transfer and launch to the International Space Station from Europe's Spaceport in Kourou, French ...

Titan's subsurface reservoirs modify methane rainfall

20 hours ago

(Phys.org) —The international Cassini mission has revealed hundreds of lakes and seas spread across the icy surface of Saturn's moon Titan, mostly in its polar regions. These lakes are filled not with water ...

User comments : 9

Adjust slider to filter visible comments by rank

Display comments: newest first

Husky
not rated yet Oct 27, 2010
The moon and earth may have a canceled out gravity tug at the lagrange points, but i would be interested to know what happens to atomic clocks/time dilation at these points?
PinkElephant
5 / 5 (4) Oct 27, 2010
@Husky,

Good question. First, there is always some degree of time dilation because we're all embedded in the gravitational well of the Sun, of our Galaxy, of our galactic super cluster, and so on. This is always in effect, as a kind of semi-constant background. But let's ignore it, for simplicity.

Secondly, theory says that time dilation in gravitational fields is a consequence of gravitational acceleration. (In other words, it occurs only in accelerated frames of reference.) The more acceleration, the more time dilation. Interestingly, there should be effectively no added time dilation at the center of the Earth, while dilation should be maximized at Earth's surface -- at least according to GR.

Lastly, at Lagrange points you aren't stationary: you're still orbiting the Earth. In all cases, your total time dilation (relative to an infinitely distant inertial observer) is always a function of both your speed and the magnitude of your acceleration.
GSwift7
5 / 5 (1) Oct 28, 2010
Yes, Pink is correct. It's called shell theory:

http://en.wikiped..._theorem

Also, as Pink pointed out, the gravity at a lagrangian point doesn't actually cancel out to zero. To understand it it helps to simplify the system down to only the Earth and Moon, and remember that the moon doesn't actually orbit the Earth exactly. In reality, the Earth and Moon are a bound pair which both orbit their shared center of gravity. The lagrangian point is where a very small object can also orbit that shared center of gravity between the two large objects. The satellite in the lagrangian point is not actually floating in zero gravity, it's in a kind of geostationary orbit around the Earth/Moon center of gravity.

As to the notion of finding a place where all gravity is actually canceled out on a universal scale, where you would have zero time dilation, there may be no such place 'inside' the universe. That's one of those big cosmology questions they agonize over.
Skeptic_Heretic
5 / 5 (3) Oct 28, 2010
As to the notion of finding a place where all gravity is actually canceled out on a universal scale, where you would have zero time dilation, there may be no such place 'inside' the universe. That's one of those big cosmology questions they agonize over.
Effectively there can't be a place of no gravity, at least not at this time. In order to have no gravitational interaction, you'd have to exist in an empty universe, but even then you'd be under the influence of your own microgravity.
GSwift7
not rated yet Oct 28, 2010
Yes, quantum physics argues that such a point of zero mass/energy density is impossible because if such a point exists in the universe then the quantum state at such a point would be exactly zero, and quantum theory says that can't happen. At least that's how I understand what I've read. ...If quantum theory is complete enough to apply it to cosmological questions?
PinkElephant
5 / 5 (2) Oct 28, 2010
@GSwift7,
In reality, the Earth and Moon are a bound pair which both orbit their shared center of gravity.
True, although the Moon's mass is tiny compared to Earth's, and that common center of gravity is actually inside the Earth's surface.
The lagrangian point is where a very small object can also orbit that shared center of gravity between the two large objects.
False: not a single one of the Lagrange points coincides with the center of gravity. For instance, see here:

http://en.wikiped...ated.gif

The center of gravity is actually a bistable local peak in gravitational potential: should you place an object there, even a tiniest perturbation of the object's position will send it plummeting toward one of the co-orbiting bodies.
GSwift7
5 / 5 (1) Oct 28, 2010
Pink, read what I said again. You misunderstood what I said. I did not say that the lagrangian point IS the center of gravity. I said that the lagrangian point orbits the center of gravity. It follows the two large bodies around the center of gravity of the two large bodies. Yes, I know where the center of gravity is between the earth and the moon. Of course, as I said before, reducing this to a three-body system is helpful for illustrative purposes, but in reality, many other factors play in. I wasn't trying to correct you. Just expanding on what you said and saying some of the same things in different wording. Stop jumping on my case for no reason. I had the courtesy to actually read your post and I agree with everything you said. I didn't say anything that disagrees with what you said, and if you read my post more carefully, you'll see that I did explain it correctly.
PinkElephant
not rated yet Oct 28, 2010
@GSwift7,

Ok, I see what you were trying to say.

I was confused by the phrase "The lagrangian point is where a very small object can also orbit that shared center of gravity". The wording seemed to imply that either the barycenter is coincident with a Lagrangian point (since objects parked at Lagrangians actually "orbit" the Lagrangian point), or that objects can orbit the barycenter *only* at Lagrange points (whereas in reality there's an infinite variety of possible orbits around the barycenter.) The latter being more obvious, I assumed you meant the former.
douglas2
not rated yet Oct 31, 2010
time dilation is a function of the gravitational potential, not the field. The dilation does not cancel at the center of mass, or at any lagrange point, in fact it is greatest at the center of gravity, the bottom of the potential well.