Nine years ago today, Dawn set sail on an epic journey of discovery and adventure. The intrepid explorer has sailed the cosmic seas and collected treasures that far exceeded anything anticipated or even hoped for. It began its voyage at Earth with a fiery ascent atop a Delta rocket. After escaping from its home planet’s gravitational grasp, it flew through the solar system perched on a pillar of blue-green xenon ions that enabled the probe to accomplish a mission that would have been impossible with conventional propulsion. In 2009, with its sights set on more distant lands, Dawn swept past Mars, taking some of the planet’s orbital energy for its own. By its fourth anniversary, Dawn was conducting an extensive orbital investigation of protoplanet Vesta, the second most massive resident of the main asteroid belt. Dawn found it to be quite unlike typical asteroids. Rather than a big chunk of rock, Vesta is like a small planet, and scientists recognize it as being more closely related to the rocky planets of the inner solar system (including Earth) than to the much smaller asteroids. Vesta’s nearer brethren are the blue and white planet where Dawn began its mission nine years ago and the red one it flew by 17 months later. By its fifth anniversary of leaving Earth, the interplanetary spaceship was on its way to yet another distant, alien world. Under the careful guidance of its human colleagues, Dawn completed its 2.5-year journey from Vesta to Ceres last year. Now a perpetual companion of the first dwarf discovered, the veteran space traveler will spend all future anniversaries in orbit around Ceres, even after its operational lifetime has concluded.
This simulated view of Ahuna Mons, Ceres’ highest mountain, was made with bonus stereo pictures Dawn acquired from an altitude of 240 miles (385 kilometers). Ahuna Mons is likely a cryovolcano (“cold volcano”), formed by cryomagma composed of salty mud rising from underground. The volcano is geologically young, probably between 50 and 240 million years. (We discussed in May how ages are estimated, but the analysis for Ahuna Mons cannot yet pin down the age more accurately.) As Ceres is nearly 4.6 billion years old, a structure that developed so recently suggests that some of the conditions that were necessary may persist even today. (So far, scientists have identified no other cryovolcanoes on Ceres.) It took somewhere between a few hundred and few hundred thousand years for the volcano to build up to its present size. The elevation of the summit is about 13,000 feet (4,000 meters), and the mountain is 11 miles (17 kilometers) across at the base. Note the streaks from rockfalls down the steep slopes (about 35 degrees). This view is from the north, and in the foreground is a crater coincidentally 11 miles (17 kilometers) across. From the lowest point in this crater to the top of the volcano is 24,800 feet (7,560 meters) vertically across a horizontal distance of only nine miles (15 kilometers). With 2.7 percent of Earth’s gravity, this could be a very nice extraterrestrial hike.
One year ago today, the ship was in its third Ceres mapping orbit, scrutinizing the exotic landscapes 915 miles (1,470 kilometers) beneath it. Less than four weeks later, it started powering its way down through the uncharted depths of Ceres gravitational field to undertake the final planned observations of its long mission.
When ion thrusting concluded on Dec. 13, 2015, Dawn was orbiting closer to Ceres than the International Space Station is to Earth. From its vantage point only 240 miles (385 kilometers) high, the probe used its suite of sophisticated sensors to develop a richly detailed portrait of the only dwarf planet in the inner solar system. Dawn’s reason for venturing to its fourth mapping orbit was to collect about 35 days of neutron spectra, 35 days of gamma-ray spectra and 20 days of gravity measurements. Given the complexity of operating in the low, tight orbit, mission planners expected it could take about three months to acquire these precious data and transmit them to Earth. Operations turned out to be essentially flawless, and by the time Dawn left that orbit on Sept. 2, it had accumulated 183 days of neutron spectra, 183 days of gamma-ray spectra and 165 days of gravity measurements. In addition, the spacecraft amassed a sensational bonus of 38,000 high resolution photos (including stereo and color) as well as more than 11 million infrared spectra and 12 million spectra in visible wavelengths. The original plan was not to take any pictures or visible or infrared spectra at the lowest altitude.
For such an overachiever, it’s fitting that now, on its ninth anniversary, the spacecraft is engaged in activities entirely unimagined on its eighth. With the critical loss of two of the four reaction wheels used to orient and stabilize the ship in space, the flight team (and your correspondent) considered it unlikely Dawn would survive long enough to celebrate a ninth anniversary. And everyone was confident that whether it was operating or not, it would still be in the fourth mapping orbit. There was a clear intent never to go anywhere else. But as we explained last month, with the extraordinary wealth of information Dawn gleaned, the team has been developing plans for new and previously unforeseen work at higher altitudes. Next month, we will detail the first set of new observations from an orbital perch of about 920 miles (1,480 kilometers).
For now, Dawn is using its ion engine #2 to gradually raise its orbit. We have seen how the spacecraft’s uniquely capable propulsion system leads to intriguing spiral trajectories. Right now, on the ninth anniversary of the last moment Dawn’s rocket stood motionless at Cape Canaveral’s Space Launch Complex 17B, Dawn is 660 miles (1,060 kilometers) above Ceres. With its signature combination of exceptional gentleness and exceptional efficiency, the ion engine will propel Dawn to an altitude 20 miles (35 kilometers) higher by the end of the day today. (In contrast, by the end of the day it launched nine years ago, Dawn had gained about 175,000 miles, or 280,000 kilometers, in altitude. The Delta rocket provided a much stronger thrust at much lower efficiency. We will discuss this further below.)
KSC / NASA
Launch of Dawn
Dawn launched at dawn (7:34 a.m. EDT) from Cape Canaveral Air Force Station, Sept. 27, 2007. Note the sun rising on the left edge of the picture. The intricate sequence of activities between the time this photo was taken and Dawn’s separation from the rocket to fly on its own is described here.
You can follow Dawn’s ascent to its new orbit by flying right behind it as it loops around Ceres or by checking the frequent mission status reports.
Nine years after launch, as Dawn maneuvers in orbit around a distant dwarf planet in order to conduct new observations, it is convenient to look back over its long trek through deep space. For those who would like to track the probe’s progress in the same terms used on past anniversaries, we present here the ninth annual summary, reusing text from previous years with updates where appropriate. Readers who wish to reflect upon Dawn’s ambitious journey may find it helpful to compare this material with the Dawn Journals from its first,second,third,fourth,fifth, sixth, seventh and eighth anniversaries.
In its nine years of interplanetary travels, the spacecraft has thrust for a total of 2,044 days (5.6 years), or 62 percent of the time (and 0.000000041 percent 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 890 pounds (404 kilograms) of its supply of xenon propellant, which was 937 pounds (425 kilograms) on Sept. 27, 2007. The spacecraft has used 68 of the 71 gallons (256 of the 270 liters) of xenon it carried when it rode its rocket from Earth into space.
The thrusting since then has achieved the equivalent of accelerating the probe by 24,800 mph (39,900 kilometers per hour). As previous logs have described (see here for one of the more extensive discussions), 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. Dawn has far exceeded the velocity change achieved by any other spacecraft under its own power. (For a comparison with probes that enter orbit around Mars, refer to this earlier log.) It is remarkable that Dawn’s ion propulsion system has provided 97 percent of the change in speed that the entire Delta rocket provided.
NASA / JPL-Caltech / UCLA / MPS / DLR / IDA
Dawn had this view on June 1, 2016, from an altitude of 240 miles (385 kilometers). It is northeast of the scene we saw earlier this year of Kupalo Crater. Kupalo is relatively young, and the impact that formed it ejected material that blanketed the surrounding area, muting the appearance of the older crater shown here. There are few craters visible in this picture because there has not been enough time since the Kupalo impact for the steady but slow rain of interplanetary debris to excavate many new craters. We saw some examples of this in pictures in April and discussed it further in May. Full image and caption.
Since launch, our readers who have remained on or near Earth have completed nine revolutions around the sun, covering 56.6 AU (5.3 billion miles, or 8.5 billion kilometers). Orbiting farther from the sun, and thus moving at a more leisurely pace, Dawn has traveled 38.6 AU (3.6 billion miles, or 5.8 billion kilometers). As it climbed away from the sun, up the solar system hill, to match its orbit to that of Vesta, it continued to slow down to Vesta’s speed. It had to go even slower to perform its graceful rendezvous with Ceres. In the nine years since Dawn began its voyage, Vesta has traveled only 36.6 AU (3.4 billion miles, or 5.5 billion kilometers), and the even more sedate Ceres has gone 34.0 AU (3.2 billion miles, or 5.1 billion kilometers). (To develop a feeling for the relative speeds, you might reread this paragraph while paying attention to only one set of units, whether you choose AU, miles, or kilometers. Ignore the other two scales so you can focus on the differences in distance among Earth, Dawn, Vesta and Ceres over the nine years. You will see that as the strength of the sun’s gravitational grip weakens at greater distance, the corresponding orbital speed decreases.)
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. (If you prefer not to skip it, click here.) In order to make the table below comprehensible (and to fulfill our commitment of environmental responsibility), we recycle some more text here on the nature of orbits.
Orbits are ellipses (like flattened circles, or ovals in which the ends are of equal size). So as members of the solar system family (including Earth, Vesta, Ceres and Dawn) follow their paths around the sun, they sometimes move closer and sometimes move farther from it.
NASA / JPL-Caltech
Dawn’s interplanetary trajectory (in blue). The dates in white show Dawn’s location every Sept. 27, starting on Earth in 2007. Note that Earth returns to the same location, taking one year to complete each revolution around the sun. When Dawn is farther from the sun, it orbits more slowly, so the distance from one Sept. 27 to the next is shorter. In addition to seeing Dawn’s progress on this figure on previous anniversaries of launch, we have seen it other times as well, most recently in July. (And, to answer an important question raised last month, this image, along with others, also will be seen for a short time this afternoon on a yummy chocolate cake at the Dawn flight team’s novennial celebration.)
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 (known as the ecliptic) is a good reference. Other planets and interplanetary spacecraft may travel in orbits that are tipped at some angle to that. The angle between the ecliptic and the plane of another body’s orbit around the sun is the inclination of that orbit. 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 ecliptic, and part of the arduousness of Dawn’s journey has been changing the inclination of its orbit, an energetically expensive task.)
Now we can see how Dawn has done by considering the size and shape (together expressed by the minimum and maximum distances from the sun) and inclination of its orbit on each of its anniversaries. (Experts readily recognize that there is more to describing an orbit than these parameters. Our policy remains that we link to the experts’ websites when their readership extends to one more elliptical galaxy than ours does.)
The table below shows what the orbit would have been if the spacecraft had terminated ion 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 Sept. 27, 2007, its orbit around the sun was exactly Earth’s orbit. After launch, it was in its own solar orbit.
Minimum distance from the Sun (AU)
Maximum distance from the Sun (AU)
Dawn’s orbit on Sept. 27, 2007 (before launch)
Dawn’s orbit on Sept. 27, 2007 (after launch)
Dawn’s orbit on Sept. 27, 2008
Dawn’s orbit on Sept. 27, 2009
Dawn’s orbit on Sept. 27, 2010
Dawn’s orbit on Sept. 27, 2011
Dawn’s orbit on Sept. 27, 2012
Dawn’s orbit on Sept. 27, 2013
Dawn’s orbit on Sept. 27, 2014
Dawn’s orbit on Sept. 27, 2015
Dawn’s orbit on Sept. 27, 2016
For readers who are not overwhelmed by the number of numbers, investing the effort to study the table may help to demonstrate how Dawn patiently transformed its orbit during the course of its mission. Note that five years ago, the spacecraft’s path around the sun was exactly the same as Vesta’s. Achieving that perfect match was, of course, the objective of the long flight that started in the same solar orbit as Earth, and that is how Dawn managed to slip into orbit around Vesta. While simply flying by it would have been far easier, matching orbits with Vesta required the exceptional capability of the ion propulsion system. Without that technology, NASA’s Discovery Program would not have been able to afford a mission to explore the massive protoplanet in such detail. But now, Dawn has gone even beyond that. Having discovered so many of Vesta’s secrets, the stalwart adventurer left it behind in 2012. No other spacecraft has ever escaped from orbit around one distant solar system object to travel to and orbit still another extraterrestrial destination. Dawn devoted another 2.5 years to reshaping and tilting its orbit even more so that now it is identical to Ceres’. Once again, that was essential to the intricate celestial choreography in March 2015, when the behemoth tenderly took hold of the spacecraft. They have been performing an elegant pas de deux ever since.
NASA / JPL-Caltech / UCLA / MPS / DLR / IDA
Water ice in Oxo Crater
This shows where Dawn’s infrared mapping spectrometer detected water ice in Oxo Crater. The crater is 6 miles (10 kilometers) in diameter. This view was constructed from bonus photographs Dawn took from an altitude of 240 miles (385 kilometers). Blue, green and infrared pictures were combined with stereo pictures to provide this perspective. (Colors are enhanced to bring out subtle differences your eye would not otherwise detect, and the vertical scale has been exaggerated by a factor of two.) Compare this with the Oxo Crater photograph shown in the April Dawn Journal. Here, we are looking from the upper left of that photo toward the lower right. Full image and caption.
Its ion propulsion system has allowed Dawn to do even more than orbit two distant and fascinating bodies. At each one, the spacecraft has changed its orbits extensively, optimizing its views to conduct detailed studies, something it would not have been able to do with conventional propulsion.
Dawn passed a coincidental pair of milestones in its orbital mission at Ceres last week. The dwarf planet reached out to take Earth’s emissary into a gentle but permanent gravitational embrace on March 6, 2015. Sept. 23, 2016, was 1,500 Cerean days later. (Ceres turns on its axis in 9 hours, 4 minutes, considerably faster than Earth, although not all that different from the giant planet Jupiter, which takes 9 hours, 56 minutes). Interestingly, on Sept. 22, Dawn completed its 1,500th orbital revolution around Ceres.
Given the equality between the number of orbits and the number of Cerean days, you may be tempted to conclude that Dawn orbits at the same rate that Ceres rotates. Please resist this temptation! Dawn’s early orbits took weeks to complete, and as the spacecraft maneuvered to lower altitudes, eventually they took days and then hours. In its lowest altitude, the spacecraft circled Ceres in only 5.4 hours. (For a reminder of the details of the orbits, see this table and this diagram depicting preliminary orbit sizes.) So, it truly is a coincidence that the average has worked out so that Dawn has revolved as many times as Ceres has rotated. And now that Dawn is raising its altitude and thus increasing the time required to complete an orbit, such a coincidence will not occur again. Ceres is very stubborn and will keep rotating at the same rate. Dawn, much nimbler and more flexible, is currently in a 13-hour orbit. By the time it completes ion thrusting next week, the orbit period will be almost 19 hours.
NASA / JPL-Caltech / UCLA / MPS / DLR / IDA
Topographical map of Ceres
This topographical map of Ceres was made from Dawn’s stereo photos taken in the third mapping orbit. (For experts, the topography is referenced to an ellipsoid of 299.5 by 299.5 by 277.1 miles, or 482.0 by 482.0 by 446.0 kilometers.) The dwarf planet is 1.1 million square miles (2.8 million square kilometers). That’s about 36 percent of the land area of the contiguous United States, or the combined land areas of France, Germany, Italy, Norway, Spain, Sweden and the United Kingdom. The map shows all the feature names approved so far by the International Astronomical Union (IAU). (We described the naming convention here.) As more features are named, this official list and map are kept up to date. (To avoid confusion, note that the topographical map here has the prime meridian on the left, but the IAU map has it in the middle.) The scales for horizontal distance in this figure apply at the equator. Rectangular maps like this distort distances at other latitudes. A similar version of this map is here.
Now in the 10th year of its deep-space expedition, Dawn is not satisfied simply to rest on its laurels. The explorer (along with its support team on distant Earth) is committed to remaining as prolific and profitable at Ceres as it was during earlier years of its extraordinary and innovative mission of discovery. The largest body between Mars and Jupiter is a relict from the dawn of the solar system, a strange and fascinating world of rock, ice and salt that likely has been geologically active for more than 4.5 billion years. Ceres was first glimpsed from Earth more than 200 years ago but held her secrets close until Earth finally answered her cosmic invitation. Now, after so very long, Ceres is whispering those wondrous secrets to her permanent companion. Dawn is listening carefully!
Dawn is 660 miles (1,060 kilometers) from Ceres. It is also 1.99 AU (185 million miles, or 297 million kilometers) from Earth, or 760 times as far as the moon and 1.98 times as far as the sun today. Radio signals, traveling at the universal limit of the speed of light, take 33 minutes to make the round trip.
Dr. Marc D. Rayman 4:34 a.m. PDT September 27, 2016