17 Nov
2014

Dawn Soars at 2014 JPL Open House

by Dawn EPO
 

Two days…
…200+ scientists and engineers…
…Live demonstrations…
…NASA’s thrilling space science.

What happens when people come together with a common mission to tell the stories of NASA and make it happen? 45,716 visitors traveled from afar to find out at the 2014 JPL Open House in Pasadena, California on October 11-12. The event, themed “Welcome to Our Universe,” invited visitors on a “ride” through the wonders of space. Highlights included a life-size model of the Curiosity rover and demonstrations from numerous space missions—including Dawn. Dawn visited giant asteroid Vesta from 2011 to 2012, and will arrive at dwarf planet Ceres in the spring of 2015. A 3-D print of protoplanet Vesta, gorgeous images, and an ion engine just like the one being used by Dawn to orbit its destinations helped the mission’s scientists and engineers tell the tale of the science, technology, engineering and mathematics (STEM) that drives the mission!

JPL Open house
Dawn team members and volunteers manned the Dawn booth answering a myriad of questions from curious space enthusiasts about NASA’s Dawn mission:

My favorite part of Open House is always seeing amazement in people’s eyes. Profound new understandings of the nature of the universe or the extraordinary power of human ingenuity register in them—it almost feels as if you participate in someone’s wonderful life-changing experience.
Marc Rayman, Chief Engineer and Mission Director of the Dawn mission

…I had one woman tell me that she’s taken a picture in front of the Dawn display every year that we’ve been at open house!
Kristina Larson, Dawn Spacecraft Systems Engineer, JPL

I was particularly surprised at how passionate people still are about Pluto’s status as a dwarf planet.
Keri Bean, Dawn Science Planning & Sequencing Engineer, JPL

People were excited to hear that Ceres was actually a planet before Pluto and that it was ‘demoted’ from planetary status to asteroid, and now ‘promoted’ to dwarf planet. They were captivated by the dynamic process of science!!
Joe Wise, Dawn EPO Lead, Wildwood School

I loved the delight and wonder in children and adults alike as they held a life-like model of Vesta, touched an ion propulsion engine, and explored a to-scale replica of the actual Dawn spacecraft. The science we’re still exploring on Vesta became real to them, the technology aboard the Dawn spacecraft awesome. We all decided we can’t wait to uncover the mysteries at dwarf planet Ceres when we arrive in spring, 2015!
Judy Counley, Dawn Education and Public Outreach

space enthusiast engaged at Dawn booth

Left: Siblings compare Ceres to other dwarf planets. Right: Brother and sister point out how colors denote elevation on the topographical map of Vesta made with stereo pictures taken by the camera aboard the Dawn spacecraft.Credit: NASA/McREL

 


 

31 Oct
2014
Marc Rayman
Marc Rayman
Chief Engineer/ Mission Director, JPL

Dawn Journal | October 31

by Marc Rayman
 

Dear Dawnomalies,

Farther from Earth and from the sun than it has ever been, Dawn is on course and on schedule for its March 2015 arrival at Ceres, an enigmatic world of rock and ice. To slip gracefully into orbit around the dwarf planet, the spacecraft has been using its uniquely capable ion propulsion system to reshape its heliocentric orbit so that it matches Ceres’ orbit. Since departing the giant protoplanet Vesta in Sep. 2012, the stalwart ship has accomplished 99.46 percent of the planned ion thrusting.

What matters most for this daring mission is its ambitious exploration of two uncharted worlds (previews  of the Ceres plan were presented from December 2013 to August 2014), but this month and next, we will consider that 0.54 percent of the thrusting Dawn did not accomplish. We begin by seeing what happened on the spacecraft and in mission control. In November we will describe the implications for the approach phase of the mission. (To skip now to some highlights of the new approach schedule, click on the word “click.”)

The story begins with radiation, which fills space. Earth’s magnetic field deflects much of it, and the atmosphere absorbs much of the rest, but there is no such protection for interplanetary spacecraft. Some particles were energized as recently as a few days earlier on the sun or uncounted millennia ago at a supernova far away in the Milky Way galaxy. Regardless of when and where it started, one particle’s cosmic journey ended on Sep. 11 at 2:27 a.m. PDT inside Earth’s robotic ambassador to the main asteroid belt. The particle penetrated one of the spacecraft panels and struck an electrical component in a unit that controls the ion propulsion system.

ion engine

Photo of ion engine thrusting in a vacuum chamber at JPL. This thrust test was on Deep Space 1, which paved the way for Dawn. Credit: NASA/JPL

At the time the burst of radiation arrived, Dawn was thrusting as usual, emitting a blue-green beam of high velocity xenon ions from engine #1. Ten times as efficient as conventional chemical propulsion, ion propulsion truly enables this unique mission to orbit two extraterrestrial destinations. With its remarkably gentle thrust, it uses xenon propellant so frugally that it takes more than three and a half days to expend just one pound (0.45 kilograms), providing acceleration with patience.

Dawn’s electronics were designed to be resistant to radiation. On this occasion, however, the particle managed to deposit its energy in such a way that it disrupted the behavior of a circuit. The control unit used that circuit to move valves in the elaborate system that transports xenon from the main tank at a pressure of 500 psi (34 times atmospheric pressure) to the ion engine, where it is regulated to around two millionths of a psi (ten million times lower than atmospheric pressure), yielding the parsimonious expenditure of propellant. The controller continued monitoring the xenon flow (along with myriad other parameters needed for the operation of the ion engine), but the valves were unable to move in response to its instructions. Thrusting continued normally for more than an hour as the xenon pressure in the engine decreased very gradually. (Everything with ion propulsion is gradual!) When it reached the minimum acceptable value, the controller executed an orderly termination of thrust and reported its status to the main spacecraft computer.

When the computer was informed that thrust had stopped, it invoked one of Dawn’s safe modes. It halted other activities, reconfigured some of the subsystems and rotated to point the main antenna to Earth.

The events to that point were virtually identical to a radiation strike that occurred more than three years earlier. Subsequent events, however, unfolded differently.

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21 Oct
2014

In Appreciation: Dr. Gerhard Neukum

by Dawn EPO
 
Dr. Gerhard Neukum

Professor of Planetary
Sciences, Freie Universität Berlin. Credit: ESA

We are remembering Gerhard Neukum today: a mentor, a friend, and a superlative colleague.

Professor Gerhard Neukum was a planetary scientist with a particular fascination for craters and the story they tell about the age and composition of a solar system body—and the solar system itself. A co-investigator on the Dawn science team, he advised with characteristic perception and tenacity.

DoubleCrater_Mar2012

Gerhard Neukum was an international expert on cratering. Double crater on giant asteroid Vesta.
Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA

Neukum’s career as a distinguished planetary scientist began in the 1970s, when he conducted research for NASA’s Apollo program as a physics student at the University of Heidelberg. Eventually he became the director of the German Aerospace Center Institute of Planetary Research before moving to the Free University of Berlin. Throughout his long and successful career he made major contributions to international space missions that visited the moon, Mars, Jupiter, Saturn, and the main asteroid belt. Neukum will always be remembered for his uncompromising determination to explore the solar system. Without his charismatic leadership, planetary science would not be where it is today.

Neukum had very high standards. He loved scientific discussions and admitted it freely when he was wrong. Amazingly this did not happen very often! Gerhard was a person you could call late at night to discuss a science issue—especially when it came to crater counting results, a particular passion.

Gerhard Neukum Image: David Ausserhofer

Gerhard Neukum Credit: David Ausserhofer

He was a great scientist who taught us about the will power to accomplish goals. Those who worked with him always appreciated his direct and energetic way of approaching and solving problems. Some did not always agree with Neukum’s outspoken way of arguing for new space missions, or the scientific details of crater counting throughout the solar system. However, everyone respected him for his intellectual capabilities and his love of exchanging fair arguments in scientific discourse.

Neukum was also the inventor of the High Resolution Stereo Camera (HRSC). With nine sensors that scan an object from a different perspective and combine the images, it pushed the boundaries of solar system imaging. A version of his camera was aboard the unsuccessful Russian Mars ’96 probe, which did not make it beyond Earth orbit. Gerhard remained undeterred. “On the plane back to Moscow,” Gerhard recalled, “I thought to myself, ‘This can’t be the end.’”1 In 2003, his camera was on board the European Space Agency’s Mars Express. Since then, scientists and citizens alike have enjoyed these sharp and stunning images.

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27 Sep
2014
Marc Rayman
Marc Rayman
Chief Engineer/ Mission Director, JPL

Dawn Journal | September 27

by Marc Rayman
 

Dear Dawnniversaries,

On the seventh anniversary of embarking upon its extraordinary extraterrestrial expedition, the Dawn spacecraft is far from the planet where its journey began. While Earth has completed its repetitive loops around the sun seven times, its ambassador to the cosmos has had a much more varied itinerary. On most of its anniversaries, including this one, it reshapes its orbit around the sun, aiming for some of the last uncharted worlds in the inner solar system. (It also zipped past the oft-visited Mars, robbing the red planet of some of its orbital energy to help fling the spacecraft on to the more distant main asteroid belt.) It spent its fourth anniversary exploring the giant protoplanet Vesta, the second most massive object in the asteroid belt, revealing a fascinating, complex, alien place more akin to Earth and the other terrestrial planets than to typical asteroids. This anniversary is the last it will spend sailing on the celestial seas. By its eighth, it will be at its new, permanent home, dwarf planet Ceres.

The mysterious world of rock and ice is the first dwarf planet discovered (129 years before Pluto) and the largest body between the sun and Pluto that a spacecraft has not yet visited. Dawn will take up residence there so it can conduct a detailed investigation, recording pictures and other data not only for scientists but for everyone who has ever gazed up at the night sky in wonder, everyone who is curious about the nature of the universe, everyone who feels the burning passion for adventure and the insatiable hunger for knowledge and everyone who longs to know the cosmos.

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31 Aug
2014
Marc Rayman
Marc Rayman
Chief Engineer/ Mission Director, JPL

Dawn Journal | August 31

by Marc Rayman
 

Dear Omnipodawnt Readers,

Dawn draws ever closer to the mysterious Ceres, the largest body between the sun and Pluto not yet visited by a probe from Earth. The spacecraft is continuing to climb outward from the sun atop a blue-green beam of xenon ions from its uniquely efficient ion propulsion system. The constant, gentle thrust is reshaping its solar orbit so that by March 2015, it will arrive at the first dwarf planet ever discovered. Once in orbit, it will undertake an ambitious exploration of the exotic world of ice and rock that has been glimpsed only from afar for more than two centuries.

An important characteristic of this interplanetary expedition is that Dawn can linger at its destinations, conducting extensive observations. Since December, we have presented overviews of all the phases of the mission at Ceres save one. (In addition, questions posted by readers each month, occasionally combined with an answer, have helped elucidate some of the interesting features of the mission.) We have described how Dawn will approach its gargantuan new home (with an equatorial diameter of more than 600 miles, or 975 kilometers) and slip into orbit with the elegance of a celestial dancer. The spacecraft will unveil the previously unseen sights with its suite of sophisticated sensors from progressively lower altitude orbits, starting at 8,400 miles (13,500 kilometers), then from survey orbit at 2,730 miles (4,400 kilometers), and then from the misleadingly named high altitude mapping orbit (HAMO) only 910 miles (1,470 kilometers) away. To travel from one orbit to another, it will use its extraordinary ion propulsion system to spiral lower and lower and lower. This month, we look at the final phase of the long mission, as Dawn dives down to the low altitude mapping orbit (LAMO) at 230 miles (375 kilometers). We will also consider what future awaits our intrepid adventurer after it has accomplished the daring plans at Ceres.

From HAMO to LAMO

Dawn’s spiral transfer from HAMO to LAMO. The trajectory turns from blue to red as time progresses during the two months. Red dashed sections are where ion thrusting is stopped so the spacecraft can point its main antenna to Earth. Credit: NASA/JPL

It will take the patient and tireless robot two months to descend from HAMO to LAMO, winding in tighter and tighter loops as it goes. By the time it has completed the 160 revolutions needed to reach LAMO, Dawn will be circling Ceres every 5.5 hours. (Ceres rotates on its own axis in 9.1 hours.) The spacecraft will be so close that Ceres will appear as large as a soccer ball seen from less than seven inches (17 centimeters) away. In contrast, Earth will be so remote that the dwarf planet would look to terrestrial observers no larger than a soccer ball from as far as 170 miles (270 kilometers). Dawn will have a uniquely fabulous view.

As in the higher orbits, Dawn will scrutinize Ceres with all of its scientific instruments, returning pictures and other information to eager Earthlings. The camera and visible and infrared mapping spectrometer (VIR) will reveal greater detail than ever on the appearance and the mineralogical composition of the strange landscape. Indeed, the photos will be four times sharper than those from HAMO (and well over 800 times better than the best we have now from Hubble Space Telescope). But just as in LAMO at Vesta, the priority will be on three other sets of measurements which probe even beneath the surface.

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31 Jul
2014
Marc Rayman
Marc Rayman
Chief Engineer/ Mission Director, JPL

Dawn Journal | July 31

by Marc Rayman
 

Dear Studawnts and Teachers,

Patient and persistent, silent and alone, Dawn is continuing its extraordinary extraterrestrial expedition. Flying through the main asteroid belt between Mars and Jupiter, the spacecraft is using its advanced ion propulsion system to travel from Vesta, the giant protoplanet it unveiled in 2011 and 2012, to Ceres, the dwarf planet it will reach in about eight months.

Most of these logs since December have presented previews of the ambitious plan for entering orbit and operating at Ceres to discover the secrets this alien world has held since the dawn of the solar system. We will continue with the previews next month. But now with Dawn three quarters of the way from Vesta to Ceres, let’s check in on the progress of the mission, both on the spacecraft and in mission control at JPL.

The mission is going extremely well. Thank you for asking.

For readers who want more details, read on…

The spacecraft, in what is sometimes misleadingly called quiet cruise, has spent more than 97 percent of the time this year following the carefully designed ion thrust flight plan needed to reshape its solar orbit, gradually making it more and more like Ceres’ orbit around the sun. This is the key to how the ship can so elegantly enter into orbit around the massive body even with the delicate thrust, never greater than the weight of a single sheet of paper.

The probe is equipped with three ion engines, although it only uses one at a time. (The locations of the engines were revealed shortly after launch when the spacecraft was too far from Earth for the information to be exploited for tawdry sensationalism.) Despite the disciplined and rigorous nature of operating a spaceship in the main asteroid belt, the team enjoys adding a lighthearted touch to their work, so they refer to the engines by the zany names #1, #2, and #3.

Dawn & TIE Fighter comparison

Artist’s comparison of Dawn spacecraft and Star Wars TIE Fighter.
Credit: NASA/JPL

Darth Vader and his Empire cohorts in “Star Wars” flew TIE (Twin Ion Engine) Fighters in their battles against Luke Skywalker and others in the Rebel Alliance. Outfitted with three ion engines, Dawn does the TIE Fighters one better. We should acknowledge, however, that the design of the TIE Fighters did appear to provide greater agility, perhaps at the expense of fuel efficiency. Your correspondent would concur that when you are trying to destroy your enemy while dodging blasts from his laser cannons, economy of propellant consumption probably shouldn’t be your highest priority.

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30 Jun
2014
Marc Rayman
Marc Rayman
Chief Engineer/ Mission Director, JPL

Dawn Journal | June 30

by Marc Rayman
 

Dear Mastodawns,

Deep in the main asteroid belt, between Mars and Jupiter, far from Earth, far from the sun, far now even from the giant protoplanet Vesta that it orbited for 14 months, Dawn flies with its sights set on dwarf planet Ceres. Using the uniquely efficient, whisper-like thrust of its remarkable ion propulsion system, the interplanetary adventurer is making good progress toward its rendezvous with the uncharted, alien world in about nine months.

Dawn’s ambitious mission of exploration will require it to carry out a complex plan at Ceres. In December, we had a preview of the “approach phase,” and in January, we saw how the high velocity beam of xenon ions will let the ship slip smoothly into Ceres’s gravitational embrace. We followed that with a description in February of the first of four orbital phases (with the delightfully irreverent name RC3), in which the probe will scrutinize the exotic landscape from an altitude of 8,400 miles (13,500 kilometers). We saw in April how the spacecraft will take advantage of the extraordinary maneuverability of ion propulsion to spiral from one observation orbit to another, each one lower than the one before, and each one affording a more detailed view of the exotic world of rock and ice. The second orbit, at an altitude of about 2,730 miles (4,400 kilometers), known to insiders (like you, faithful reader) as “survey orbit,” was the topic of our preview in May. This month, we will have an overview of the plan for the third and penultimate orbital phase, the “high altitude mapping orbit” (HAMO).

(The origins of the names of the phases are based on ancient ideas, and the reasons are, or should be, lost in the mists of time. Readers should avoid trying to infer anything at all meaningful in the designations. After some careful consideration, your correspondent chose to use the same names the Dawn team uses rather than create more helpful descriptors for the purposes of these logs. What is important is not what the different orbits are called but rather what amazing new discoveries each one enables.)

It will take Dawn almost six weeks to descend to HAMO, where it will be 910 miles (1,470 kilometers) high, or three times closer to the mysterious surface than in survey orbit. As we have seen before, a lower orbit, whether around Ceres, Earth, the sun, or the Milky Way galaxy, means greater orbital velocity to balance the stronger gravitational grip. In HAMO, the spacecraft will complete each loop around Ceres in 19 hours, only one quarter of the time it will take in survey orbit.

Sprial to Hamo

Dawn’s spiral descent from survey orbit to the high altitude mapping orbit. The trajectory progresses from blue to red over the course of the six weeks. The red dashed segments are where the spacecraft is not thrusting with its ion propulsion system (as explained in April). Credit: NASA/JPL

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31 May
2014
Marc Rayman
Marc Rayman
Chief Engineer/ Mission Director, JPL

Dawn Journal | May 31

by Marc Rayman
 

Dear Dawnosaurs,

Silently streaking through the main asteroid belt, emitting a blue-green beam of xenon ions, Dawn continues its ambitious interplanetary expedition. On behalf of creatures on distant Earth who seek not only knowledge and insight but also bold adventure, the spacecraft is heading toward its appointment with Ceres. In about 10 months, it will enter orbit around the ancient survivor from the dawn of the solar system, providing humankind with its first detailed view of a dwarf planet.

This month we continue with the preview of how Dawn will explore Ceres. In December we focused on the “approach phase,” and in January we described how the craft spirals gracefully into orbit with its extraordinary ion propulsion system. The plans for the first observational orbit (with a marvelously evocative name for a first examination of an uncharted world: RC3 — is that cool, or what?), at an altitude of 8,400 miles (13,500 kilometers), were presented in FebruaryLast month, we followed Dawn on its spiral descent from each orbital altitude to the next, with progressively lower orbits providing better views than the ones before. Now we can look ahead to the second orbital phase, survey orbit.

Survey_orbit

This figure shows Dawn’s second observational orbit, “survey orbit,” at the same scale as the size of Ceres. At an altitude of 2,730 miles (4,400 kilometers), the spacecraft will make seven revolutions in about three weeks. Credit: NASA/JPL

In survey orbit, Dawn will make seven revolutions at an altitude of about 2,730 miles (4,400 kilometers). At that distance, each orbit will take three days and three hours. Mission planners chose an orbit period close to what they used for survey orbit at Vesta, allowing them to take advantage of many of the patterns in the complex choreography they had already developed. Dawn performed it so beautifully that it provides an excellent basis for the Ceres encore. Of course, there are some adjustments, mostly in the interest of husbanding precious hydrazine propellant in the wake of the loss of two of the spacecraft’s four reaction wheels. (Although such a loss could have dire consequences for some missions, the resourceful Dawn team has devised a plan that can achieve all of the original objectives regardless of the condition of the reaction wheels.)

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29 May
2014

Greetings From Berlin–Grüße aus Berlin!

by Chris Russell
 

The Dawn Team Converges at the German Aerospace Agency

The Dawn spacecraft moved back in solar system time when it cruised into the main asteroid belt, first orbiting protoplanet Vesta in 2011-12, and now on its way to dwarf planet Ceres, due in March 2015. When the Dawn team met in Berlin this month, it offered an opportunity for the mission to do a bit of its own time travel.

Dawn Team at the German Aerospace Agency, Berlin, 2014

fig 1: Dawn Team at the German Aerospace Agency, Berlin, 2014

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23 May
2014

Vesta 360

by David O'Brien
 

The Dawn mission is currently en route to dwarf planet Ceres, its second destination. It spent a productive fourteen months orbiting its first destination, giant asteroid Vesta, in 2011-12, gathering splendid sets of data. The spacecraft may have moved on, but the science team continues to explore that data, enriching our understanding of Vesta’s formation and history.

Getting the “Big Picture”

Vesta: Clementine color ratios

Clementine color ratios

Vesta is a large protoplanet with remarkably variable topography—mountains, troughs, boulders, craters, cliffs, and more. The wealth of high-resolution imaging data from the Dawn mission has given us an amazing view of its surface. However, looking through individual frames or image mosaics can make it difficult to see its surface features in a global context and get the “big picture” of Vesta. On the other hand, the images taken early on as the mission approached the protoplanet show the whole of Vesta, but with low surface resolution. To better visualize Vesta at high resolution, I used the open-source program POV-Ray[1], combining images and topography data to create striking 3-D graphics.

The program let me take a shape model of Vesta, created from Dawn’s framing camera data by Bob Gaskell at the Planetary Science Institute, and wrap an image around it. For the image, I used a global mosaic[2] developed by our framing camera team partners at the German Aerospace Center (DLR) from high altitude mapping orbit clear-filter images. This mosaic has a resolution of 60 meters (about 200 feet) per pixel. I then used POV-Ray to make ‘snapshots’ of this model of Vesta as it rotated, varying the latitude from +45 to -45 degrees. Those individual frames were combined into the movie shown below.

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Footnotes:
  1. [1] Persistence of Vision Raytracer
  2. [2] The global mosaics used here can be downloaded from this page at the Dawn Public Data website, although they are very large files. For labeled maps of smaller regions of the surface, see the Vesta Atlas.