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The red dot at the center of this image is the first near-Earth asteroid discovered by NASA's Wide-Field Infrared Survey Explorer, or WISE -- an all-sky mapping infrared mission designed to see all sorts of cosmic objects. Image credit: NASA/JPL-Caltech/U

We have discovered our first new near-Earth asteroid with WISE. Our first "golden ticket" is now known as 2010 AB78. It's an asteroid that is roughly 1 kilometer [about .6 miles] in diameter, so it's fairly large. The most interesting thing about it so far is that we thought we knew of about 85 percent of all the asteroids 1 kilometer and larger, so finding a big one like this is a little unusual. Of course, unlike Charlie and his chocolate bars, finding the golden ticket wasn't a matter of luck, but a meticulous search process more like a busy assembly line.

Near-Earth objects are asteroids and comets with orbits that get close to Earth's orbit. That doesn't mean they are going to hit the Earth, of course. It's sort of like driving on a busy street; just because there are a lot of cars zipping by on either side of you, it doesn't necessarily mean your car is going to hit one. The cars would have to be at the same place at the same time for that to happen. So even though the paths each car has traveled might get close, there is no collision.

WISE finds asteroids by using a sophisticated piece of software called the WISE Moving Object Processing System, or WMOPS. When we first get a set of images from WISE, we have software that automatically searches the images for all the sources in them, be they stars, galaxies or asteroids. The software records their positions and how bright they are. WMOPS goes into that source list and figures out which sources are moving compared to the fixed stars and galaxies in each frame. Then, it figures out which sources are actually the same object -- just observed at different times. So it's a pretty smart piece of code. The whole system has to be highly automated, since when the WISE survey is done, the source catalog will contain several hundred million sources! You can imagine that trying to sort through all of these to find individual objects would be very challenging without a nifty program like WMOPS.

Our newest addition to the approximately 6,600 near-Earth Asteroids that are currently known is shown in this new image above.

2010 AB78 shows up like a glowing red ember at the center of the image, because it's glowing brightly in infrared light with a wavelength of 12 microns, which is about 20 times redder than your eye can see. The stars appear blue, because they're much hotter, and they emit proportionally less of their energy at these long wavelengths. The color that the asteroids appear to WISE is an important feature we use to distinguish them from other stars and galaxies, in addition to their motion.

With this first asteroid discovery, we are flexing our muscles in preparation for the heavy lifting we're about to start.


  • Amy Mainzer

Artist concept of NASA's Dawn spacecraft

Dear Dawnters and Sons,

The Dawn mission continues to go smoothly, as Earth’s distant envoy carries out its interplanetary journey. Although the craft still devotes most of its time to the slow but efficient reshaping of its orbit around the Sun to match Vesta’s, controllers gave it some extra assignments since the last log to ensure its systems remain healthy and to prepare for its studies of Vesta.

Dawn usually interrupts ion thrusting once a week for about 8 hours to point its main antenna to Earth. On November 30, however, instead of resuming thrusting, it dutifully followed different instructions that were stored onboard.

The spacecraft began the 5 days of special activities by activating the gamma ray and neutron detector (GRaND). Despite its name, GRaND is not at all pretentious, but its capabilities are quite impressive. It will reveal the atomic constituents of the surfaces of Vesta and Ceres. GRaND’s measurements of space radiation this month showed it to be in excellent health. After a week of smooth operation, it was deactivated on December 7.

The visible and infrared mapping spectrometer (VIR) and the primary science camera also were turned on for the first time in more than half a year. As these sensors yield complementary data, controllers want to refine earlier measurements of exactly how their views overlap. This will allow scientists to correlate observations from the instruments in order to glean as much as possible about the nature of the protoplanets the craft will orbit. Dawn rotated to point at a star and then observed it simultaneously with VIR and the camera. By measuring precisely where the star registers in each device, their relative alignments can be pinned down. Upon completing the sequence of commands to acquire the desired data, the spacecraft turned to point its main antenna to Earth again and began transmitting the results during the next scheduled session with the Deep Space Network a few hours later.

The VIR team quickly discovered that a subtle incompatibility between certain instructions in the program for recording the signals from the star caused its shutter to remain closed. (VIR also has a reusable protective cover, but that operated as intended.) The unit continued to function and stayed healthy, but it did not perform the planned observations. The science camera imaged the target, but the purpose was to compare where the star appeared in the 2 instruments. The VIR commands are easily corrected, and the calibration will be executed again early next year.

Earlier this year, engineers developed new software for the science camera to improve its efficiency in mapping the distant worlds Vesta and Ceres. The software was updated once before in space, and the process followed this week was the same. As last year, loading software into the primary and the backup cameras was performed as entirely separate activities; each camera was off while the other was being upgraded. This was the only major work this week that was not accomplished with commands that had previously been stored on the spacecraft. After the new software was installed, each camera was directed to carry out a set of tests, and the results confirmed that both were operating correctly.

Among the other tasks this week was an annual evaluation of the backup star tracker, a device that recognizes star patterns so the spacecraft can calculate its orientation. To verify that the tracker remained healthy, the unit was powered on and operated. It correctly took pictures, identified the stars, and then determined the direction it was pointed. The tests verified that the unit remains in good condition and ready to be called into service in the unlikely event a problem with the primary tracker occurs.

On December 4, after completing all of its scheduled activities for the week, Dawn turned once again to point ion thruster #1 in the direction needed for propelling itself to Vesta, and resumed emitting high-speed xenon ions. It has continued since then with its familiar schedule of quiet cruise.

As the effect of the thrust continues to build up, tomorrow Dawn will pass another milestone. The thrusting since the beginning of the mission will have achieved the equivalent of accelerating the spacecraft by 2.00 miles per second (3.22 kilometers per second, or 7200 miles per hour). This is well in excess of what most spacecraft accomplish with their propulsion systems but is less than 1/3 of the planned maneuvering for the mission. To achieve this extraordinary velocity, Dawn has expended less than 126 kg (278 pounds) of xenon propellant during 474 days of powered flight. While the day-to-day change is small (as we will discuss in greater detail in February), with 24 hours of thrusting yielding just 7.2 meters per second (16 miles per hour), the benefit of its acclaimed patience is becoming evident.

As we have discussed several times (see, for example, this previous log), Dawn’s actual speed has not changed by the values just presented. In the complex orbital dance it performs, partnered principally by the Sun but with others joining in as well (Mars being the most significant this year), the more it thrusts and climbs away from the Sun, the slower it travels. Nevertheless, the equivalent change in speed (that is, the change that would be achieved in the absence of the complications from being in orbit) is a handy measure of the effect of any spacecraft’s maneuvering.

While Dawn continues pushing away from the Sun and deeper into the asteroid belt, the distance to Earth is still declining, as it has been since November 2008. The separation between the planet and the probe varies just as the distance between the tips of the hour hand and minute hand increases and decreases every hour. That suggests that it’s time once again to refer to one of the clocks available in the Dawn gift shop on your planet. (If you didn't get around to preparing for the recent festivities marking the universe's reaching its present age, don't despair. Although there are only 5 trillion shopping days until the next such gala celebration, Dawn gift shops in most galaxies are offering attractive discounts right now.)

To picture the changing alignment, let’s recall the clock described 365 days ago, with the Sun at the center. Dawn is at the tip of the minute hand and Earth is at the tip of the shorter hour hand. One year ago today, the celestial alignment corresponded to the position of the hands at about 6:01:45. At that time, Dawn was 2.49 astronomical units (AU) from Earth. In the intervening year, Earth has completed 1 orbit around the Sun, returning to where it was. Having traveled more slowly, Dawn is in a different position now that happens to be much closer to Earth. Today the alignment is similar to that at 6:30:00. Even though Dawn is farther from the Sun today than it was 1 year ago (as if the length of the minute hand had increased), in its current location around the clock face, it is 0.84 AU from Earth, only 1/3 of what it was at the end of last year. The cosmic hands will continue to move into still-closer alignment until late next month, when the Sun, Earth, and Dawn will lie nearly along a straight line.

Picturing Dawn’s position relative to Earth and the Sun may help some readers gain perspective on the explorer’s interplanetary journey, and we will continue to present such illustrations (at least as long as the increased revenue for the gift shop makes it profitable to do so). Nevertheless, it is worth bearing in mind that from Dawn’s perspective, the location of Earth is of little importance (except when it needs to point its antenna there). The ship travels on its own course around the Sun, independent of the motions of the distant celestial port from which it set sail more than 2 years ago. Dawn’s sights remain firmly fixed on the destinations ahead, where it seeks to unlock secrets about the dawn of the solar system.

Dawn is 0.84 AU (125 million kilometers or 78 million miles) from Earth, or 345 times as far as the moon and 0.85 times as far as the Sun. Radio signals, traveling at the universal limit of the speed of light, take 14 minutes to make the round trip.

Dr. Marc D. Rayman
6:30:00 pm PST December 30, 2009

› Learn more about the Dawn mission


  • Marc Rayman

Artist concept of NASA's Dawn spacecraft

Dear Dawnticlimaxes,

Dawn continues to make steady progress through the solar system as it maintains a gentle pressure on its orbit around the Sun. It has spent 95% of the time since the last log thrusting with its ion propulsion system, stopping only briefly each week to communicate with the mission control team on distant Earth.

The probe is on an exciting journey to unlock secrets from the dawn of the solar system ensconced in the mysterious worlds Vesta and Ceres. And yet there is one aspect of this expedition that likely is much less exciting than some readers may expect.

Dawn entered the main asteroid belt on November 13. As it ventures ever deeper into this vast collection of material between Mars and Jupiter, it may be tempting to think of the spacecraft constantly dodging asteroids. In some science fiction movies, the huge rocky bodies are so close together that highly skilled piloting is required to avoid catastrophes. Now Dawn is guided by some of the most proficient interplanetary fliers this side of Pluto, but the reality is that accidental impacts are exceedingly unlikely. Space is big, and as plentiful as asteroids are, the distances between them are tremendous.

After crossing the threshold of the belt earlier this month, Dawn will travel 7.7 astronomical units (AU), or nearly 1.2 billion kilometers (almost 720 million miles), to its July 2011 rendezvous with Vesta. Yet in all that time, and across all that distance, the closest the probe will come to a catalogued asteroid is 1.0 million kilometers (greater than 600 thousand miles), or more than 2.5 times the distance between Earth and the moon. Certainly travelers on Earth would not consider something that far away to be a hazard (especially compared to what many Dawn team members regularly experience on the freeways in Los Angeles), and neither would our intrepid explorer.

To bring this down to a more tractable scale, we can imagine Dawn’s journey through the asteroid belt to Vesta as a trip from New York City to Los Angeles, with rocks littered along the way. In this case, along the entire route to a bizarre and forbidding land, the nearest we would come to one of these rocks would be 3.4 kilometers (2.1 miles) -- hardly a close call. At that distance, it would be difficult even to detect the rock, as it would be a mere 1.5 centimeters (less than 5/8 of an inch) in diameter; this corresponds to an asteroid less than 5 kilometers (under 3 miles) across. Even looking out to 20 kilometers (12 miles) during our trek, the largest object we would pass would be just 3.4 centimeters (1.3 inches), representing a 10-kilometer (6-mile) asteroid Dawn will miss by 15 times the distance between Earth and the moon.

Dawn is bound for the giants of the asteroid belt. Vesta’s equatorial diameter is about 580 kilometers (360 miles), and Ceres is 975 km (605 miles) across. (Remember that when thinking about three-dimensional worlds such as these, the diameter may fail to illustrate how large they really are.) Together these two behemoths contain more than a third of all the mass in the main asteroid belt. On the scale of our cross-country drive, Vesta would be 2.0 meters (6.5 feet) wide and Ceres would be 3.3 meters (11 feet). Rather than missing them by great distances, we would move to within 0.6 meters (2 feet) of the first target and 2.4 meters (8 feet) of the second.

Dawn’s science instruments are optimized for studying these immense bodies in detail from orbit around them, just as many Earth-observation spacecraft peer down constantly on our planet. Diverting the probe to zip past a chunk of rock for a very brief view would be possible, but doing so would take precious time away from the far richer and more valuable investigations planned for Vesta. That is where Dawn will find the rewards of the next 20 months of travel.

While astronomers observe members of the asteroid belt as small as about a kilometer (a mile), what about still smaller rocks that are large enough to damage the spacecraft? Because available telescopes generally are not powerful enough to detect such objects from Earth, mathematical models are used to predict their prevalence and thus Dawn’s likelihood of encountering them. Although far more abundant than the larger asteroids, there still are too few pebbles distributed over the enormous volume of space through which the ship sails to pose a serious threat.

The spacecraft was designed so that the tiniest particles, which are sufficiently plentiful that some likely will strike it, cannot inflict significant damage. Dawn’s largest area is in its solar arrays, and asteroidal dust cracking a few of the 11,480 cells is inconsequential. More sensitive components are covered with protective materials that will cause the high-speed grains to break up and slow down before they reach the vulnerable elements. There is good reason to believe Dawn’s travels in the asteroid belt will be safe.

Even as Dawn recedes from the Sun, Earth (moving faster in its tighter solar orbit) is approaching the spacecraft; indeed, the distance has been decreasing for more than a year (and will continue to do so for another 2 months). On December 5, the craft and the star will be equidistant from the planet. We saw instances of these 3 members of the solar system family forming a triangle with 2 equal sides, known as an isosceles triangle, on May 28, 2008 and again on September 18 of this year. In those cases however, the equal sides were those between Dawn and Earth and between Dawn and the Sun. Next month, it will be Earth at the apex of the astronomical triangle, with both the spacecraft and the Sun at a distance of 0.99 AU. The third leg of the triangle, from Dawn to the Sun, will be 1.70 AU.

To illustrate the geometry, let’s use one of the new clocks that have just reached the shelves of the Dawn gift shop on your planet. (And note that for any purchase through the end of 2009, we will donate a used xenon ion to the charity of your choice.) With Earth at the center of the clock face, if the Sun were at the 10, Dawn would be the same distance but at the 2. (The clock hands are not important here; the objective is to illustrate the relative lengths and the angles of the isosceles triangle. Ignoring the hands also lets us offer the clock at a very low price!)

Any readers who happen to reside on or be visiting Earth on December 5 may find this arrangement a convenient opportunity to contemplate something of the nature of an interplanetary voyage. Dawn is quite invisible even to the most powerful telescopes, but it will be at the same distance as the most easily detectable extraterrestrial body, the Sun. The spacecraft has been more remote (as have other probes) and will be again later in the mission, but on that day it will be just as far from Earth as the star that rules from the center of the solar system. While the Sun has seemed -- indeed, has been -- unreachably distant for the overwhelming majority of human history, farther even than any horizon travelers could set their sights on, a craft that we set sail upon the cosmic ocean will be exactly that far away.

To add more dimensions to our mental imagery of Dawn’s location, we can take advantage of another celestial reference on December 6, before the triangular alignment of the previous day has changed noticeably. At about 8:30 am PST, the spacecraft will appear just over 2 degrees (or a little more than 4 times the moon’s diameter) north of the moon. As the moon’s orbit carries it around Earth, it will be less than twice that far from the apparent position of the spacecraft for the 6 hours before and after that time, so anyone who can see the moon during that interval can get a rough fix on Dawn’s location. For readers in North America, the alignment occurs when the moon is the western sky after dawn (yes!). From the vantage point of the center of the clock, observers may be able to see both the Sun and the approximate location of the spacecraft at the same distance, letting their imaginations take over where their eyes leave off. Out there, in that direction, as far as the Sun, will be Dawn, patiently, reliably, silently continuing its bold voyage of exploration.

Dawn is 1.03 AU (154 million kilometers or 96 million miles) from Earth, or 395 times as far as the moon and 1.05 times as far as the Sun. Radio signals, traveling at the universal limit of the speed of light, take 17 minutes to make the round trip.

Dr. Marc D. Rayman
4:30 pm PST November 27, 2009

› Learn more about the Dawn mission


  • Marc Rayman

Artist's concept of the Wide-field Infrared Survey Explorer. Image credit: NASA/JPL-Caltech

Now that we are just days from launch (wow!), the team is making final decisions and preparations. We've just held our Flight Readiness Review, at which the final commitment to launch was made by NASA, the United Launch Alliance (the rocket folks) and the WISE project. It turns out that fueling our Delta II rocket's second stage engine is an irreversible process -- once we fuel the second stage, we have 34 days to launch the rocket. If we don't launch within 34 days of fueling it, we have to replace the second stage completely -- and that would mean taking WISE off the rocket. So we needed to be really sure that we were "go for launch" before we decided to fuel up the second stage. That is now done, and we are in the process of putting the final finishing touches on cooling down our solid hydrogen tanks.

These last few weeks and days before launch require a lot of flexibility of the team, since the schedule can change on a dime. There are about a million things having nothing to do with the launch vehicle or the spacecraft that can delay a launch -- winds, too much fog, too many clouds, lightning and even something as mundane as a fishing boat or aircraft straying into the "keepout" zone that's established around the launch site. You would think that the prospect of running into a giant, 330,000-pound rocket loaded with fuel would be enough to make people move out of the way, but sometimes they don't seem to get the message! Any of these items is enough to scrub a launch attempt.

But that's why we've built in the ability to make two consecutive launch attempts with WISE, separated by 24 hours. We get two tries. After that, our tank full of frozen hydrogen starts to warm up too much, and it takes two days for us to cool it back down. To keep the tank of frozen hydrogen a frosty 7 degrees above absolute zero (minus 447 Fahrenheit), we circulate an even colder refrigerant, liquid helium, around the outside of the tank. But the process of re-cooling takes two days; we have to hook all the hoses back up, cool everything down, then disconnect the hoses again before the next launch attempt.

So we have to be flexible. We've all put our lives on hold for the duration, since we have to be ready for anything that happens. Meanwhile, I've frantically tried to take care of stuff like cleaning the house and laying in supplies, because once WISE launches, things will go into overdrive. Needless to say, our families have all been very patient with us!


  • Amy Mainzer

Artist's concept of the Wide-field Infrared Survey Explorer. Image credit: NASA/JPL-Caltech

With WISE a mere month away from liftoff, it's probably a little late to be asking why we need to send it into space. But it's worth taking the time to explain why we go to all the trouble of sending something up on a rocket. While it's really cool to go into space, we're not just sending WISE up there for the fun of it. In this case, there's no other reasonable way to accomplish the mission's science goals: surveying the entire sky in infrared, finding the nearest star to our sun, and finding the most luminous galaxy in the universe. We can't do this from the ground.

It turns out that the main culprit that drives us into space and into an orbit more than 500 kilometers (about 360 miles) above the Earth's surface is our atmosphere. As wonderful as our atmosphere is for life on Earth, it wreaks havoc on astronomical images in many ways. For one, shifting pockets of warm and cool air drifting above a telescope -- or a human observer-- cause stars to twinkle. While pretty, this twinkling makes it difficult to get a good measurement of a star's true brightness (or, in astronomical terms, its "photometry"). The twinkling also reduces the telescope's sensitivity and resolution by enlarging the images it produces, making them blurrier and less sharp. This is true for all kinds of telescopes not just infrared ones.

Secondly, the atmosphere acts like a sponge at many wavelengths, soaking up light from the stars so that it never reaches the ground at all. Everybody's seen a rainbow at one time or another, and that range of colors -- from violet to red -- spans the maximum range of wavelengths that our eyes can see. But that is only a small fraction of the entire spectrum of light that's really out there in the universe. Our sun puts out most of its radiation in visible light, and most of that visible light makes it through our atmosphere to the ground. However, our atmosphere is only partially transparent to infrared wavelengths. Filled with water vapor, carbon dioxide, and methane, our atmosphere absorbs almost all infrared light, so most of the infrared light emitted by distant stars, asteroids, and planets doesn't make it to observers on the ground. These molecules grab infrared light and trap it, preventing it from passing through the atmosphere (which is why they are called greenhouse gases). To see anything at all in most infrared colors, we have to get entirely above the Earth's atmosphere.

The final problem posed by our atmosphere for infrared astronomers is that it -- and the Earth itself -- is warm. Infrared light is characteristically emitted by room-temperature objects. Objects like you and I glow brightly in infrared light, and so does the Earth and its atmosphere. If you could see in infrared light, the night sky would look as bright as daylight! So when we're trying to detect the faint heat signatures of distant astronomical objects, a glowing, warm atmosphere is almost impossible to see through. This is why we must cool the WISE telescope to a mere 12 degrees above absolute zero (minus 438 Fahrenheit). Being in space with a cold telescope makes such a huge difference that the relatively modest-size WISE telescope, which is 40 centimeters (16 inches) in diameter, is equivalent in sensitivity to literally thousands of 8-meter (26-foot) telescopes on the ground. That small WISE telescope packs a punch.

So with that cleared up, we're just about ready to put WISE into the nose cone and crane it up onto the Delta II rocket that's waiting for us on the launch pad. Let's go see some stars!


  • Amy Mainzer

Artist concept of NASA's Dawn spacecraft

Dear Dawn-o’-lanterns,

Dawn continues to make steady progress on its journey through the solar system. The spacecraft has devoted another month to thrusting with its ion propulsion system, ever with its sights set on its rendezvous with Vesta in July 2011. While it will have other assignments along the way, propelling itself to the giant protoplanet deep in the main asteroid belt remains its principal responsibility.

The asteroid belt consists of innumerable objects in orbit around the Sun between Mars and Jupiter. (Dawn is aiming for the 2 most massive members of the belt.) Just as with a ball of cotton or a cloud, while there may appear to be a clear border when viewed from a great distance, a more careful examination reveals it to be less distinct. There is no sharp edge to demarcate the boundary. For example, although most asteroids remain between the two planets, the orbits of some bring them closer to the Sun than Mars. We can adopt a part of one common definition in which, to be designated as a resident of the main asteroid belt, an object’s orbit can bring it no closer to the Sun than 1.666 astronomical units (AU). It is not coincidental that this is the greatest distance that Mars travels from the Sun. (Earth and its inhabitants never reach more than 1.017 AU from the solar system’s gravitational master.)

As with Earth, Mars, and asteroids, Dawn’s orbit around the Sun is elliptical. The principal difference is that the ship is constantly changing its course by emitting a high velocity beam of xenon ions. (It has racked up more than 10,000 hours of powered flight, with much more thrusting ahead.) In a lovely solar system dance in February, Dawn briefly partnered with Mars for additional assistance on its way as well. As we saw in the last log, the spacecraft’s orbit grows larger as the mission progresses, bringing the explorer ever closer to its first destination. On November 13, it will enter the asteroid belt as its silent flight takes it past 1.666 AU from the Sun. It will remain in the belt for the rest of its mission and well beyond. Dawn will become a permanent inhabitant of that part of the solar system, the first emissary from Earth to take up residence in the main asteroid belt.

The probe has been here before. On June 30, 2008 it passed the outermost part of Mars’s orbit. But its elliptical path reached its greatest distance from the Sun of more than 1.68 AU on August 8, 2008, and 40 days after that, it crossed the orbit of Mars again. On April 17, 2009, then at 1.37 AU from the Sun, its momentum began carrying it outwards once again. By then it was in a larger orbit, and thanks to the extensive additional orbital energy imparted to the spacecraft by its persistent ion thrusting, it will sail smoothly through 1.68 AU next month and continue deeper into the asteroid belt.

As Dawn continuously enlarges its solar orbit still more, mission controllers work diligently to ensure the distant craft remains healthy. They are also preparing to give it some additional tasks before the year is out, and inside sources reveal that these may be described in an upcoming log. In the meantime, emitting its eerie bluish glow, the probe silently streaks toward unexplored worlds, seeking to reveal new secrets and likely new questions as well.

Dawn is 1.25 AU (187 million kilometers or 116 million miles) from Earth, or 485 times as far as the moon and 1.26 times as far as the Sun. Radio signals, traveling at the universal limit of the speed of light, take 21 minutes to make the round trip.

Dr. Marc D. Rayman
11:30 pm PDT October 31, 2009

P.S. Although Dawn works tirelessly in interplanetary space, the team on Earth is taking a break for Halloween. Observant readers have already noticed that this correspondent has dawned his costume, and it is a delightful and impressive disguise indeed. In an act of astonishing creativity, he is pretending to be someone who can write a (relatively) short log.

› Learn more about the Dawn mission


  • Marc Rayman

Artist concept of NASA's Dawn spacecraft

Dear Dawnniversaries,

Dawn is celebrating the second anniversary of leaving its home planet by engaging in the same function it has performed most of its time in space: with the utmost patience, it is using its ion propulsion system to gradually modify its orbit around the Sun.

In its interplanetary travels, the spacecraft has thrust for a total of about 389 days, or 53% of the time (and about 0.000000008% of the time since the Big Bang). While for most spacecraft, firing a thruster to change course is a special event, it is Dawn’s wont. All this thrusting has cost the craft only 103 kilograms (228 pounds) of its supply of xenon propellant, which was 425 kilograms (937 pounds) on September 27, 2007.

The thrusting so far in the mission has achieved the equivalent of accelerating the probe by 2.62 kilometers per second (5870 miles per hour). As previous logs have described, because of the principles of motion for orbital flight, whether around the Sun or any other gravitating body, Dawn is not actually traveling this much faster than when it launched. But the effective change in speed remains a useful measure of the effect of any spacecraft’s propulsive work. Having accomplished only one-fifth of the thrust time planned for its entire mission, Dawn has already far exceeded the velocity change achieved by most spacecraft. (For a comparison with probes that enter orbit around Mars, refer to a previous log.)

Since launch, our readers who have remained on or near Earth have completed 2 revolutions around the Sun, covering about 1.88 billion kilometers (1.17 billion miles). Orbiting farther from the Sun, and moving at a more leisurely pace, Dawn has traveled 1.57 billion kilometers (980 million miles). As it climbs away from the Sun to match its orbit to that of Vesta, it will continue to slow down to Vesta’s speed. Since Dawn’s launch, Vesta has traveled only 1.18 billion kilometers (730 million miles).

Readers with nothing better to do have already discovered that much of the text in the 3 preceding paragraphs is taken verbatim from the log that commemorated Dawn’s first anniversary of being in space, with the principal changes being that the numbers are updated here. (In addition, most of the humor was removed to comply with a request from the Glum Legion of Ardent Dawnniversaries). This is not a result of any more otiosity than normally displayed by your correspondent; rather, comparing the beginning of this log with last year’s may be helpful for measuring the progress in the intervening time. Of course, most of the last 12 months was devoted to coasting, and the gravitational boost from Mars is not reflected in the effect of the ion thrusting, but the comparison may be illuminating for some readers. This also provides a handy preview of the beginning of the September 27, 2010 log. [Note to self: Perhaps there really is an option here for greater lassitude. Think about that after taking a nap.]

Another way to investigate the progress of the mission is to chart how Dawn’s orbit around the Sun has changed. This discussion will culminate with a few more numbers than we usually include, and readers who prefer not to indulge may skip this material, leaving that much more for the grateful Numerivores.

Orbits are ellipses (like flattened circles, or ovals in which the ends are of equal size). So as members of the solar system family follow their paths around the Sun, they sometimes move closer and sometimes move farther from it. For thinking about these distances, we may remind ourselves once again of the convenient unit of measure in the solar system, the astronomical unit (AU).

In addition to orbits being characterized by shape, or equivalently by the amount of flattening (that is, the deviation from being a perfect circle), and by size, they may be described in part by how they are oriented in space. Using the bias of terrestrial astronomers, the plane of Earth’s orbit around the Sun is a good reference. Other planets and interplanetary spacecraft travel in orbits that are tipped at some angle to that. Vesta and Ceres do not orbit the Sun in the same plane that Earth does, and Dawn must match its orbit to that of its targets. (The major planets orbit closer to the plane of Earth’s orbit, and no spacecraft has had to venture as far out of that plane to orbit another body as Dawn will.)

Now we can see how Dawn has been doing by considering the size and shape (together expressed by the minimum and maximum distances from the Sun) and the angle of its orbit on its anniversaries. (Experts readily recognize that there is more to describing an orbit than these parameters. Our policy is to link to the experts’ sites when their readership extends to 1 more elliptical galaxy than ours does.)

The table below shows what the orbit would be if the spacecraft terminated thrusting on its anniversaries; the orbits of its destinations, Vesta and Ceres, are included for comparison. Of course, when Dawn was on the launch pad on September 27, 2007, its orbit around the Sun was exactly Earth’s orbit. After launch, it had its own orbit.

Minimum distance from the Sun (AU) Maximum distance from the Sun (AU) Angle from Earth’s orbit
Dawn’s orbit on Sept. 27, 2007 (before launch) 0.98 1.02 0.0°
Dawn’s orbit on Sept. 27, 2007 (after launch) 1.00 1.62 0.6°
Dawn’s orbit on Sept. 27, 2008 1.21 1.68 1.4°
Dawn’s orbit on Sept. 27, 2009 1.42 1.87 6.2°
Vesta’s orbit 2.15 2.57 7.1°
Ceres’s orbit 2.54 2.99 10.6°

Readers may disregard the table or gaze into it for insight or inspiration for as long as they like. The point of it, however, is to illustrate both that Dawn has come a long way since the launch pad, and it has a long journey ahead before it begins its exploration of Vesta.

But the trek will be a little shorter than mission planners had anticipated until quite recently. As we have seen in a previous log, the plan for thrusting depends on how much electrical power will be available to the ion propulsion system, which converts electrical power into thrusting power. Greater electrical power translates into higher (but still exceptionally gentle) thrust.

Last year Dawn’s engineers, who remain on distant Earth, devised a method to calibrate the solar arrays, and the spacecraft dutifully carried it out. The resulting data, combined with an extensive refinement of the mathematical model that predicts solar array power, allowed the team to be confident in increasing the prediction of the future availability of power by up to 10%. Equipped with this crucial information, they could update the plan for thrusting.

Many other factors affect the design of the thrust profile as well. As one example, how effective the thrust is depends on how massive the spacecraft is. Although weightless, Dawn still has mass (the resistance to a change in its velocity), and the greater the mass, the lower the acceleration provided by the ion thruster. This phenomenon is no different from what readers experience frequently even in the gravity of their home planet. The heavier the load you carry, the more gradually you will accelerate, whether the effort is exerted by the muscles in your legs (or wings or tentacles, depending on your species) or the engine in your car (or spaceship). Dawn’s mass decreases as the mission progresses because the ion propulsion system expends xenon and the reaction control system expends hydrazine. By refining predictions for how much of these propellants will be onboard at all times for the rest of the mission, engineers could predict how long it will take Dawn to propel itself into the same orbit around the Sun as Vesta and then later into the same orbit as Ceres.

After an extended set of analyses late in 2008 and the first half of 2009, all the elements needed to update the thrust plan were in place. The seemingly modest improvement in solar array power is by far the dominant one. When all were combined, the result revealed that Dawn’s remarkable maneuvering capability over the course of the mission will be even better than engineers had been counting on. The probe will be able to reach Vesta about 6 weeks earlier than had previously been planned. Moreover, the newfound capability will enable the craft to travel from Vesta to Ceres more quickly, so the deadline for leaving the first world to reach the second on schedule in 2015 is about 6 weeks later.

Together, these changes allow the explorer to increase its planned 9-month stay at Vesta to 12 months. This is of extraordinary benefit to the project. Vesta promises to be a fascinating place to visit, and we know quite well from other solar system adventures that no matter how much data we collect, there is always still more to learn. Mission planners had been working hard to squeeze as much as possible into the precious time they expected Dawn could spend at Vesta, so being able to increase the duration of its residency there by a third makes a tremendous difference. As details continue to be formulated for all the activities necessary to operate at and study this alien world, the additional time will prove extremely valuable in allowing the team to accommodate the glitches that are inevitable in such a complex expedition and to uncover as much of Vesta’s intriguing story as possible.

Dawn is already following the new flight plan, targeting where Vesta will be in July 2011. It is not enough, though, just for them to be in (nearly) the same place at the same time. That would result in a flyby, but our probe will enter orbit around the protoplanet, accompanying it on its orbit around the Sun, just as satellites of Earth remain close by throughout the planet’s solar orbit. The craft will remain with Vesta until July 2012, when it will begin thrusting to Ceres. We have discussed before why flying by (providing only a glimpse of each body) is significantly less challenging than matching orbits (enabling more extensive explorations), a capability that would be essentially impossible without the ion propulsion system. A subsequent log will delve further into this issue, as it is a fundamental feature of this ambitious mission.

As Dawn begins its third year in space, now on its new and better course, much work remains before it can return the scientific bounty it seeks. We hope readers will continue to follow the progress of this bold adventure in the exciting years to come.

Dawn is 1.50 AU (225 million kilometers or 140 million miles) from Earth, or 555 times as far as the moon and 1.50 times as far as the Sun. Radio signals, traveling at the universal limit of the speed of light, take 25 minutes to make the round trip.

Dr. Marc D. Rayman
4:34 am PDT September 27, 2009

P.S. The astronomical unit has been mentioned in these logs frequently enough that we will include that convenient unit of measurement from now on in the famously unimaginative concluding paragraph. It might appear redundant to present the distance from Earth both in astronomical units and in terms of how many times as far as the Sun it is. Isn’t that simply 2 different ways to describe exactly the same quantity? Well, no it is not; they are different, although they are close. An astronomical unit is the average distance between Earth and the Sun and hence does not change. The actual distance varies slightly throughout the year, so Earth’s distance from the Sun at any given time may not be precisely the average value of 1.00000000 AU (149,597,871 kilometers or 92,955,629 miles). This would be more apparent if your correspondent did not round off the numbers as dramatically. The details on that closing text are that Dawn is 1.50456971 AU (225,080,425 kilometers or 139,858,224 miles) from Earth. At the same time, Earth is 1.00222102 AU (149,928,510 kilometers or 93,161,078 miles) from the Sun, very close to the average, but not exactly equal to it. So Dawn is 1.50123544 times as far from Earth as the Sun is, given the distance to the Sun now. When rounded off, the distance in astronomical units and the distance in terms of how far the Sun is both come out to 1.50, but we see they are not really equal. Other times of the year, when the actual distance to the Sun is farther from the average, the difference will be apparent. As long as these secrets of the final paragraph are being revealed, here are the rest: the distance relative to the moon is rounded to the nearest multiple of 5, and the travel time for radio signals to the nearest minute. But just for this special occasion: Dawn is 556.865373 times as far as the moon right now, and radio signals take 25 minutes 1.574966 seconds. Approximately. Best regards to the Numerivores.

› Learn more about the Dawn mission


  • Marc Rayman

Artist concept of NASA's Dawn spacecraft

Dear Indawnmitables,

The Dawn mission remains on course as the spacecraft continues to thrust with its ion propulsion system, patiently, persistently, and gently changing its orbit to keep its appointment with protoplanet Vesta in two years. Meanwhile, closer to mission control and in stark contrast, brave firefighters work hard to protect JPL and the nearby homes of many of its employees and others in the community.

The probe has continued in “quiet cruise” since the last log. During this month, engineers did give the robot a few extra tasks to ensure it remains healthy, but these were routine. When each such assignment was conducted the first time or two that Dawn was in space, they were treated as special activities, with even greater diligence than is normally applied to the unforgiving and complex undertaking of flying a spacecraft far from Earth. Now however, the commands for these activities are stored onboard well ahead of time along with the routine commands for thrusting, communicating with Earth, and carrying out all the other functions the spacecraft normally conducts without the mission control team devoting extra attention.

Included in the maintenance procedures were instructions to perform a sequence of movements of the mechanism that points ion thruster #1, to power off reaction wheel #2 and return #1 to service, and to operate the gyroscopes for about 4 days. For readers who do not have their copies of the Dawn operations manuals handy, some information about these 3 kinds of operations was provided in a previous log.

Another event that is now considered routine occurred on August 15. For the second time this year, a particle of space radiation struck a particularly sensitive electrical component on the spacecraft, depositing enough energy to interfere with the operation of a circuit. When this happened in January 2008, it caused Dawn to enter safe mode, interrupting its other activities. Thanks to software the team transmitted to the ship later that year, now the interplanetary explorer is immune to strikes in that formerly vulnerable location.

As Dawn continues its long (in space and in time) solar system journey to match orbits with Vesta and later with Ceres, both of which reside farther from the Sun than the probe has yet traveled, some readers may note a surprising trend in the statistics for the mission. The famously unimaginative ending of each of these logs reveals that Dawn’s distance from Earth has been diminishing since November 2008. Indeed, the probe’s maximum separation from its planet of origin occurred on November 10. Today, it is as far from Earth as it was on June 2, 2008. By January 2010, it will be as close as it was in March 2008. Is this progress?

Earth and Dawn, each following its own path, are both in orbit around the Sun. As grateful residents of the planet know, their world’s orbit doesn’t change very much. The planet keeps following the same nearly circular path around the Sun year after year after year. Today Earth is about 1.01 astronomical units (AU) from the Sun, and it never strays very far from its average distance of 1.00 AU. As Dawn has traveled independently of Earth, thanks to the push from its Delta rocket, its orbit has been farther from the Sun than Earth’s. The gradual effect of ion thrusting and the much more abrupt boost from Mars have caused that orbit to change considerably since then. To enter orbit around Vesta, Dawn will have to match the giant asteroid’s orbit around the Sun, ranging from 2.15 AU to 2.57 AU. Today, Dawn is 1.53 AU from the Sun and headed outward.

As we saw a year ago (that is, one Earth-orbit-around-the-Sun ago), objects at different orbital distances travel at different speeds. The probe, orbiting the Sun at a greater range than Earth, travels more slowly, because the Sun’s gravitational attraction diminishes with distance. So as Dawn heads slowly for Vesta, gradually spiraling away from the Sun, and Earth speeds around more quickly in its orbit, sometimes our planet moves closer to the spacecraft and sometimes it moves farther away.

In a continuing effort to offset the extraordinary cost of these logs with the handsome revenue from subtle product placements, we can refer to still another in the apparently endless line of Dawn clocks (many of which have been described in recent logs and all of which are available in the Dawn gift shop on your planet). On this clock, the minute hand is shorter than the hour hand. The motion of the former represents Earth, traveling closer to the Sun (at the clock’s center) and more quickly. Dawn is at the tip of the hour hand, moving more slowly in its larger orbit. (We’ll ignore for now that the hour hand should be growing in length, as the spacecraft recedes from the Sun.) Some of the time (such as between noon and about 12:30), the distance between the ends of the hands increases, but then the situation reverses; the faster minute hand begins moving closer and closer to the hour hand as the time approaches about 1:05.

Earth and Dawn are exhibiting the same repetitive behavior, albeit more complicated because of Dawn’s ever-changing orbital speed and distance from the Sun. They will continue to draw closer until January, when Earth, coming from behind, passes Dawn and moves on ahead. The explorer will not need to take note however, as its sights are set on the asteroid belt.

So for readers tracking the distances reported in each log, don’t despair. The continuously declining separation between Earth and its celestial envoy is a reflection of the elegant mechanics of the cosmos and not the result of inattentive engineers setting the spacecraft on the wrong path.

Next month, as Earth and the spacecraft continue their separate solar system dances, together with the Sun they will briefly make an attractive arrangement. On September 18, Dawn will be just as far from the Sun as it is from Earth, at 1.56 AU from each. Earth and the Sun will be 1.00 AU apart. The trio formed a very similar pleasing pattern last year. A triangle such as this, with two sides of equal length, is usually called “isosceles.”

Although there is nothing inherently significant for the mission about this alignment, we can use one more clock example to illustrate this isosceles triangle. In this case, we put Dawn at the center and Earth at the 12. (This clock may not be as useful for telling time as some of the others that are available, but it would still make a great gift.) The Sun would be next to the sixth little tick mark, where the minute hand would point at about 6 minutes and 15 seconds after the hour. (Note that this depiction of the geometry illustrates the angles and the relative separations of Dawn, Earth, and the Sun; hence, the clock may be any size. Several sizes are available in the gift shop, and we helpfully recommend the most expensive one.)

Not only is Dawn on course for the asteroid belt, on course for returning new and exciting discoveries from its enigmatic destinations, it is on a new and better course than it had been. According to inside sources, the vast team of writers specifically assigned to create the next log is already planning to explain what has changed and why. Just as all loyal readers, your correspondent is hoping for an interesting description of this improvement in the mission.

Dawn is 250 million kilometers (156 million miles) from Earth, or 620 times as far as the moon and 1.66 times as far as the Sun. Radio signals, traveling at the universal limit of the speed of light, take 28 minutes to make the round trip.

Dr. Marc D. Rayman
10:30 pm PDT August 30, 2009

› Learn more about the Dawn mission


  • Marc Rayman

Artist concept of NASA's Dawn spacecraft

Dear Indawnfatigables,

Shhhh! Dawn is in “quiet cruise,” and we do not want to disturb it. The indefatigable spacecraft is devoting most of its time to thrusting with its ion propulsion system, applying a gentle but persistent pressure to its trajectory around the Sun. With patience, it will reshape its orbit to match those of the mysterious and intriguing protoplanets Vesta and Ceres. In order to conduct its detailed explorations of each of these exotic worlds, Dawn will accompany them around the Sun, visiting with Vesta in 2011 - 2012 and rendezvousing with Ceres in 2015.

Today Dawn is 220 million kilometers (137 million miles) from the star at the solar system’s center. We can express this more conveniently by recalling the ruler so often used in describing interplanetary distances, the astronomical unit (AU). The average distance between Earth and the Sun, nearly 150 million kilometers (93 million miles), is defined to be 1 AU. (For comparison, Mars, whose orbit is not as circular as Earth’s, travels between about 1.38 AU and 1.67 AU.) Today Dawn is 1.47 AU from the star at the solar system’s center.

If the spacecraft stopped thrusting now, well, gosh, that would be a disappointment! But let’s calm down and think about it anyway. Its momentum would keep it going around the Sun in an elliptical orbit that ranged from about 1.38 AU to 1.84 AU. Vesta, the first stop on Dawn’s solar system itinerary, lives between 2.15 AU and 2.57 AU. Dawn has a lot of work left to do!

The task is far more difficult than simply enlarging its orbit to have precisely the same shape as Vesta’s. In addition, Dawn has to change the orientation of its orbit so it overlaps Vesta’s. Even that is not sufficient, however, because the spacecraft also has to be in the same place in its orbit that Vesta is in its. It wouldn’t be helpful to be on exactly the same path but be very far apart.

Still, let’s consider just the problem of changing the size of the orbit. If Dawn thrust all day today but stopped tomorrow, the one day’s worth of work would change the orbit by only about 0.0004 AU. For another perspective on the effect of the thrusting, compare the orbit size 2 paragraphs above with the orbit Dawn was in after the boost from Mars. The difference is the result of 7 weeks of powered flight, yet on the scale of these vast distances, it is so small it barely registers. Yes, there is indeed a great deal of work ahead.

Dawn will reach Vesta in about 2 years. The key to getting there is the combination of the extraordinary efficiency of the ion propulsion system with the patience and reliability of all systems. The probe’s persistence in quiet cruise will pay off with the excitement of its discoveries in the asteroid belt.

Now why is this deemed “quiet cruise”? It’s true that in space no one can hear you thrust, but that’s not the reason. Rather, it is considered quiet because the spacecraft is not engaging in any special routines or functions (assuming you don’t consider traveling for years in deep space to be special). Thrusting is Dawn’s most familiar activity. Even with the long coast from October 31, 2008 to June 8, Dawn has spent about half of its time since launch tirelessly adjusting its orbit. In contrast, the great preponderance of spacecraft coast all of the time (or nearly so), just as planets and asteroids do, simply going where their orbits take them.

Dawn has already had plenty of time in space that was not quiet (readers of these logs have shared in some such times), and much more lies ahead, particularly when it is in orbit around its two very distant targets. For now though, the spacecraft’s focus is on its trek to Vesta. While its engineering colleagues will continue to be diligent in maintaining Dawn’s health and providing regular updates to its flight plan, the quiet cruise does afford the team more time to develop and refine plans for operations at Vesta. A great deal of work remains to prepare for that not-so-quiet time.

But really, how quiet is quiet cruise? In fact, Dawn is a hive of activity. For the probe to reach its targets in the asteroid belt, all engineering systems labor together. For the following discussion, reminders of the essentials of each of these systems are available by clicking here (note that this link works only for loyal readers), and another detail is available here.

For the ion propulsion system to keep emitting a steady stream of high-speed xenon ions, it must regulate the delicate flow of xenon from the main tank at more than 1000 pounds per square inch (for you readers on Earth, that’s about 70 times atmospheric pressure, and for you readers on Venus, that’s low pressure) to the thruster at roughly one millionth of a pound per square inch (around one ten-millionth of atmospheric pressure). It constantly ionizes the xenon and electrically accelerates it, requiring careful control of the high currents and voltages. The electrical power system delivers to the ion propulsion system the needed power; it supplies all other systems as well. It draws its energy from the solar array wings and converts it to the voltage its onboard customers need.

To keep the huge arrays pointed at the Sun and the ion thruster aimed in the direction needed to travel to Vesta, the attitude control system is always at work. Five times every second it takes a fix with its star tracker and computes the orientation, or “attitude,” of the craft in the void of space. If needed, it rotates the solar arrays, and it uses several different means to adjust the entire spacecraft’s attitude to achieve the required thruster pointing.

The telecommunications system continually transmits a radio signal through one of the small antennas, broadcasting a very wide beam that encompasses Earth so that mission controllers can listen in whenever they choose. The system is also unceasingly alert, listening for an almost imperceptible radio whisper from Earth in case human team members need to contact the probe between the weekly sessions that use the main antenna.

Every second the thermal control system reads more than 100 temperature sensors and decides which heaters to turn on or off to keep each component from becoming too cold or too hot.

The command and data handling system, including the main computers, is orchestrating most of this activity. It switches its attention 200 times per second as it communicates with other components. About 35 times every second it assesses all the data available from around the ship and selects some for storage and subsequent transmission to Earth through the main antenna. More than 200 parameters are checked each second so that if there are any problems, the software can take action, promptly issuing instructions to protect the craft and the mission, ensuring unexpected situations do not get out of control. And while performing these and many other functions on its own, every second the software checks to find out whether there is a stored command from mission control. Engineers formulate these directives many weeks in advance and place them onboard to be carried out at the precise second planned.

So quiet cruise really is not so quiet. And yet, this is what Dawn was designed to do. In the forbidding depths of space, all the systems work together in a near frenzy of activity to hold the stalwart ship steady, keeping it healthy and on course, as it maintains its sights on the distant horizon, where the asteroid belt beckons.

Dawn is 275 million kilometers (171 million miles) from Earth, or 710 times as far as the moon and 1.84 times as far as the Sun. Radio signals, traveling at the universal limit of the speed of light, take 31 minutes to make the round trip.

Dr. Marc D. Rayman
12:30 am PDT July 28, 2009

› Learn more about the Dawn mission


  • Marc Rayman

Artist concept of NASA's Dawn spacecraft

Dear Dawnterested Readers,

Having completed the longest planned coasting period of its entire mission, Dawn is now back to its familiar routine. On June 8, the ion propulsion system was called back into action to propel the probe to its rendezvous with asteroid Vesta.

The spacecraft began its 7-month coast period on October 31, 2008. Since then, it had used its ion thrusters for a measurement of the solar array power, a small adjustment in its course to Mars (the gravitational effect of which provided a boost to its distant destination), and tests of the software remotely installed on the main computer in April. The accumulated thrusting during all of those activities added only about 10 hours to the mission’s log of 282 days when coasting commenced.

Now that the ship has resumed its powered flight, the spacecraft devotes most of its time to thrusting. With the utmost patience, like an artist perfecting each delicate detail in a grand masterpiece, Dawn gradually reshapes its orbit around the Sun. A full day of thrusting is enough only to change its speed by a modest 7 meters/second (less than 16 miles/hour).

Dawn thrusts all but about 6 to 8 hours per week, providing only a brief opportunity to turn away from the direction it needs to aim its ion thruster in order to point its main antenna at Earth. That weekly radio communications session affords the robotic explorer its sole contact with mission controllers. While it is thrusting, Dawn is programmed to broadcast signals from one of its small, auxiliary antennas, spreading its radio signal in a wide swath that encompasses distant Earth. Usually one of the exquisitely sensitive receivers of NASA’s Deep Space Network will listen in on the spacecraft for a few hours halfway through the week, capturing the extraordinarily faint transmission showing the spacecraft is sailing smoothly.

Spending so much time thrusting is possible thanks to the extremely frugal use of xenon propellant. The ion thruster expels only about 0.26 kilograms (10 ounces) in a day. So while Dawn would need nearly 4 days to accelerate from 0 to 60 miles/hour, it would consume little more than 1 kilogram (about 2.3 pounds) of its supply of xenon during that time.

As the probe climbs away from the Sun to reach the cold depths of the asteroid belt, the multiyear thrust profile is designed to make its solar orbit match that of Vesta. The current flight plan has it arriving at the massive protoplanet in September 2011, requiring it to thrust for more than 700 days along the way, the significant majority of the time.

Prior to resuming thrust, the spacecraft carried out a routine check of one its scientific instruments. All of the instruments designed to uncloak the secrets Vesta and Ceres hold about the dawn of the solar system spend most of the time during the interplanetary cruise switched off, waiting for their opportunities to go to work in orbit. Each instrument is powered on occasionally to verify its health. On May 27, the visible and infrared mapping spectrometer (VIR) was activated. On this occasion, VIR repeated the routines it first executed in space in October 2007. All of its mechanisms were exercised, and they operated smoothly. Instead of aiming at distant celestial targets, its visible and infrared detectors measured emissions from built-in lamps. VIR passed the 4-hour test with flying colors (some of which are outside the range of human vision).

The VIR operation was one of many assignments for the coast period, most of which have been described in logs since November 2008. With all activities completed successfully, the spacecraft set about thrusting right on schedule. On June 8, executing instructions already stored in its main computer, Dawn rotated to point thruster #1 in the required direction. It powered on the ion beam shortly after 11:59 am PDT. Any readers who happened to be in the vicinity during their own deep-space excursions would immediately have recognized the familiar scene: Dawn majestically perched once again atop a blue-green pillar of xenon ions, as its ambitious journey of exploration continues.

Dawn is 291 million kilometers (181 million miles) from Earth, or 775 times as far as the moon and 1.91 times as far as the Sun. Radio signals, traveling at the universal limit of the speed of light, take 32 minutes to make the round trip.

Dr. Marc D. Rayman
5:00 am PDT June 28, 2009

› Learn more about the Dawn mission


  • Marc Rayman