The Educator Workshop was held at the same time as the Dawn Science Symposium. We were invited to the opening session.

The first speaker was Dawn Principal Investigator Dr. Chris Russell. Dr. Russell reviewed the history of the Dawn mission.
The Dawn mission was first proposed in 1994. It was originally proposed as a mission to the moon. It was not selected. The mission then changed from a lunar mission to a mission to the asteroid Vesta and then to both Vesta and Ceres. (These are the two largest asteroids.)
One unique feature of the Dawn mission is the use of an ion engine. Xenon gas “fuels” the ion engine. The xenon is ionized and is ejected out the thruster nozzle. There is a major difference in how an ion engine is used. A chemical engine is fired for seconds or minutes each time it’s fired. The ion engine can be fired for months at a time. The ion engine is more efficient and ions come out of the engine faster. This makes the engine more efficient and less fuel is required.
Dr. Russell said that an ion engine is the only way that mission could be done. Dawn will orbit Vesta and then leave Vesta orbit, travel to Ceres, and orbit Ceres. This requires enough fuel to enter the orbit of Vesta, blast out of Vesta orbit, and then enter Ceres orbit. This would require more chemical fuel than could have been placed on Dawn.
The ion engine was, in part, responsible for the Dawn mission not being selected in the late 90’s. NASA’s space probe, Deep Space One, was the first use of an ion engine on a space probe. There were problems with DS1’s ion engine. Because of these problems, Dawn was not approved.
The Dawn mission team studied the problems and modified their ion engines. They also included three thrusters. This means there are back-up engines if one fails.
The Dawn mission was approved in 2001. After a final review, Dawn was approved for launch in 2004 and set for launch in 2006. Unfortunately, Dawn was cancelled in March 2006 because of cost overruns and technical problems. Three weeks later, after protests from planetary scientists, NASA reversed the decision and Dawn was given life again. It was scheduled for a 2007 launch.

We next heard from Dr. Lucy McFadden, Co-Investigator. Dr. McFadden discussed her recent studies of Vesta using the Hubble Space Telescope. She mentioned that her study of Vest
a was the last done before the Wide Field Planetary Camera stopped working.
Vesta has a unique feature at its south pole. It appears that it was hit by a large object early in its history. Because of the impact, the south pole is not round. You can see this in this artist’s drawing of Vesta.
She also mentioned that it is believed that most meteorites on Earth originated on Vesta.
Photographs were taken over a period of two days. The purpose was to study features on Vesta’s surface. Many different features were visible in photographs. These photographs will be used to decide how to use Dawn when it orbits Vesta.
Here’s a video of Vesta rotation:
Dr. McFadden discussed what would happen when Dawn orbited Vesta and Ceres.
Dawn will begin at an altitude of about 1,500 miles to survey each asteroid. It will then drop to 500 miles to map the surface of Vesta and Ceres. Finally, it will drop to a 125-mile orbit. At this point, the Visual Infrared (VIR) Spectrometer and Gamma Ray and Neutron Detector (GRaND) will map the surface of the asteroids (more on these experiments later).

Dr. Mark Sykes, Director of the Planetary Science Institute and Dawn Co-Investigator, discussed “What is a Planet?” He discussed the recently adopted definition of a planet:
1. Is in orbit around the Sun.
2. Has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape
3. It has cleared the neighborhood around its orbit.
Dr. Sykes pointed out that that less than 500 out of 10,000 IAU members voted on the definition.
This definition is opposed by most planetary scientists. Dr. Sykes put up a photograph similar to this one.

As you can see, Mercury, Venus, Earth, Mars, and Jupiter have not cleared the neighborhood around their orbits. By this definition, these bodies should not be considered planets.
Most planetary scientists have let it be known that they will not accept this definition. They feel that only the first two definitions should be used. This would give us eleven planets instead of eight. Ceres, Pluto, and Eris would be considered planets.
In fact, he would take it one-step further and include Pluto’s moon Charon as a planet. This is because it’s round, it orbits the Sun, but it doesn’t really orbit around Pluto. If you were to look at Pluto and Charon as they orbit each other, you would see that the barycenter of their orbit is outside the surface of Pluto. They are orbiting around a point between Pluto and Charon.
You can see this in this animation from the New Horizon’s website.
This would give us twelve planets.
Later that afternoon, we had presentations from scientists who designed three of the experiments on Dawn.

Dr. Tom Prettyman discussed the Gamma Ray and Neutron Detector (GRaND). GRaND will measure the chemical composition of Vesta and Ceres.
GRaND will identify how much of each chemical, compound, etc. is found in the surface of each asteroid. It will also identify what water is present. There is a current proposal that there is a body of water or ice below the surface of Ceres. GRaND should be able to determine if the body of water or ice is there.
Knowing the composition of the asteroids will help understand how the solar system was formed. Knowing the chemical composition these asteroids will help determine the composition of the solar nebula.
GRaND data, along with data from the Visual Infrared Spectrometer and the framing camera will answer many questions about the conditions in the solar nebula that led to the formation of the solar system.

Dr. Holger Sierks, Framing Camera Project Manager, discussed the framing camera. Two cameras have been put on Dawn, ensuring that there is a back-up in case one camera fails.
The camera will have three filters – red, blue, and yellow. It looks like an old View-Master™ disk. It also has a mechanism similar to the View-Master™ to change the filter.
It will be used to help Dawn navigate as it approaches and enters orbit. Once in orbit, the Framing Camera will be used to map the surface of Ceres and Vesta.

Dr. Maria Cristina De Sanctis, Technical Manager, Instituto Nazionale di Astrofisica, discussed the Visual Infrared (VIR) spectrometer.
The VIR Spectrometer uses visual and infrared colors to determine the chemical composition and minerals found on the surface of the asteroids. Data from the VIR Spectrometer will be used along with data from GRaND and the Framing Camera to give the science team a thorough understanding of the composition and structure of Vesta and Ceres.
In addition to the briefings we received, there were breakout sessions where we had a chance to try Dawn lesson plans we can use in the classroom.
The first breakout session was a lesson about the history and discovery of the asteroids called “How Bright Are You?”
In this lesson, students are given a table with the Asteroid name, year of discovery, its maximum brightness, and its size. Students are expected to create two graphs – Asteroid Brightness vs. Year of Discovery & Size of Asteroid vs. Year of Discovery.
When students complete their first graph, they will see that, with two exceptions, the brighter the asteroid, the earlier it was discovered (four asteroids were discovered in a seven-year period. The next asteroids were discovered beginning in 1845.
The second graph shows students that, with a one exception, the first asteroids discovered were the largest.
Using the information, students expected to learn:
The larger the asteroid, the brighter it is.
The larger asteroids were discovered first.
Students complete a worksheet using their data to answer the questions.
This activity helps students learn how to analyze data and answer questions using this data.
The next session was called “Analyzing Telescopic Images.”
Students are given telescopic images of Vesta. Using those pictures, students complete the worksheet by analyzing their pictures. For example, they come up with possible explanations for the differences in brightness on Vesta’s surface and, using all pictures, they attempt to determine the direction of Vesta’s rotation as well as the tilt of its axis.
“In Search of …” required students to analyze star charts and identify where the asteroid is. They are required to identify the “star” that moved.
This activity gives students an experience similar to what earlier astronomers had to do to find an asteroid among many stars.
“Edible Rocks” required students to describe a piece of candy that had been cut. Students see a side view of the candy and then describe it, using non-food terms.
Students are then given a description of each piece of candy written by scientists that study meteors. Using those descriptions, they identify which description describes their “meteorite.”
I liked this activity because not only can I use this with my 6th grade students when we study the solar system, I can use this with my 7th grade students. 7th graders learn about classification. This activity gives them the opportunity to learn how to describe something in a way that allows others to use their description and identify the object.
The final sesson was “Design a Mission.” Students are given a NASA Discovery Program Announcement of Opportunity and required to submit a proposal.
Students receive the Discovery Program requirements and a sheet that outlines the costs of the rocket & fuel (about $80,000,000), science team, instruments, etc. Their mission can cost no more than $350,000,000.
Once done, students have to present their mission to the class. They have to name their project, design a mission patch, explain what it is going to study, identify the instruments they will use, and the total cost of the mission.
These activities give students a taste of what scientists do when they study the solar system. They develop important life skills: the ability to analyze and present data, use their knowledge in creative ways to solves problems, present their results to a group, be prepared to explain and answer questions, etc.
Having spent three days learning about Dawn, I now feel like I am a part of the Dawn mission. I have been following it very closely over the last two weeks. (I was very disappointed by the delay of the launch until September!) I will be using Dawn lessons and information about the asteroids in my science curriculum in both 6th and 7th grade.
Programs like this help teachers get a broader view of the missions NASA launches to explore the solar system. It also helps to “reinvigorate” the teacher. I came away from the workshop excited about taking what I’ve learned and using it in my curriculum. All teachers should have the chance to attend workshops like this. It helps remind us why we became science teachers!