[meteorite-list] Dawn Journal - August 31, 2016

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Wed, 21 Sep 2016 16:04:20 -0700 (PDT)
Message-ID: <201609212304.u8LN4Kit005832_at_zagami.jpl.nasa.gov>


Dawn Journal
Dr. Marc Rayman
August 31, 2016

Dear Sedawntary Readers,

Dawn is actively continuing to add details to the intimate portrait it
is creating of Ceres, a distant and exotic world. The dwarf planet has
been revealing many secrets to the companion she has held in her tender
but firm gravitational embrace since early last year.

Following the conclusion of Dawn's ambitious 8.8-year prime mission on
June 30, the spacecraft has been gathering a wealth of data with all sensors
in its extended mission as it orbits closer to Ceres than the International
Space Station is to Earth. When the adventurer descended to its current
orbital altitude of 240 miles (385 kilometers) in December 2015, mission
controllers had planned for only a few months of operations. Because of
the prior failure of two reaction wheels, used for orienting the craft
in space, Dawn had to rely on the creativity of the team to stretch the
dwindling supply of hydrazine to keep the ship operating. No one on the
team expected their efforts to be as productive as they turned out to
be, allowing the mission to continue much longer. Now Dawn has completed
more than eight months of virtually flawless activities at this altitude,
over 1,100 orbital revolutions, returning far, far more data than ever

We have recounted in recent months how Dawn has overachieved, and its
extended mission has sustained that favorable trend. As just one example,
since Ceres first showed up as a small, fuzzy blob in Dawn's camera in
December 2014, the spacecraft has taken more than 51,000 photos of Ceres
(and more than 51,000 more photos of Ceres than discoverer Giuseppe Piazzi
took). More than 37,000 of those have been taken in this fourth and lowest
orbit, providing exquisite resolution.
Dawn LAMO Image 147

Dawn had this view of Ceres' limb on May 30, 2016, from its low-altitude
mapping orbit 240 miles (385 kilometers) above the alien world. At the
bottom is Rao Crater, 7 miles (12 kilometers) in diameter. (Rao was a
god associated with the planting of turmeric for the Mangarevan people
of Polynesia.) This is one of the occasional scenic photographs of the
landscape reaching to the horizon. (We saw another last month as well.)
Full image and caption. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Dawn has achieved so much that it has been given new, special assignments
not even envisioned at the beginning of this year. For example, scientists
recently adjusted settings for the gamma ray spectrometer to search for
the signature of atoms that were not part of the original program of inventorying
Ceres' elements.

The reason for flying so low was to measure nuclear radiation and the
variations in the gravity field. In fact, Dawn was not designed to map
the vast territory with its other instruments from this tight orbit. All
the pictures, infrared spectra and visible spectra have been bonuses of
a successful mission. We have seen before how difficult it was to capture
specific geological features on Ceres with the camera. It is even more
challenging with the visible and infrared mapping spectrometers because
they share a much narrower view than the camera. Nevertheless, with great
effort, the team managed in the extended mission to obtain beautiful spectra
of the famous bright region in Occator Crater, known from earlier spectra
to be highly reflective deposits of salt left behind when briny ice covering
the ground inside the crater sublimated. Dawn has been successful in tracking
down other important sites with its visible and infrared spectrometers
as well.

After photographing more than 99.9 percent of the dwarf planet at high
resolution, the spacecraft took a great many more pictures at different
angles, making stereo views to improve the topographical map it developed
in the third mapping orbit. In addition, Dawn used the filters in its
camera to take new, sharper color photos of some of the most geologically
interesting locations.

The explorer has acquired other pictures of special scientific interest
as well. Let's delve into one kind. We have described Dawn's findings
about the location of the north and south poles and the tilt of Ceres'
rotational axis. As we saw, Earth's axis is tilted more, so our planet
experiences greater variation in the position of the sun during one heliocentric
revolution (one year). On Ceres, the sun never moves far from the equator,
which means it is always far from the poles. From the perspective of the
high northern or southern latitudes, the sun is always near the horizon
and is never high in the sky. As a result, the floors of some craters
near the poles are in shadow continuously throughout the Cerean year (which
lasts 4.6 terrestrial years). Without even brief warming rays of the distant
sun, these locations must be especially cold.
Dawn LAMO Image 153

Dawn looked down from 240 miles (385 kilometers) on May 27, 2016, at this
scene at 73 degrees north latitude. From this location, the sun (which
is off the picture, far to the right) never gets high above the horizon.
More recently, Dawn has taken long exposures to see into some of the craters
that are in persistent shadow. Full image and caption.
Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Thanks to Dawn, we know ice has been on the ground in some places in the
past and is there even now in Oxo Crater. (We also know there is a tremendous
amount of ice underground.) When ice on the surface is heated enough by
the sun, it sublimates, the water molecules receiving enough energy to
escape from the solid, becoming a gas. Some of them leave with so much
energy, they break free of Ceres' gravitational pull and go far into space.
But many of the molecules follow a familiar parabolic arc, landing elsewhere
on the dwarf planet, just as a ball thrown on Earth will come back down.
If the landing spot is similarly warm enough for ice to sublimate (as
most places on Ceres are), eventually the molecule will be lofted again,
having a chance of landing in a new, random location. But molecules that
happen to fall in the deep cold of a crater in persistent shadow will
be trapped. As a result, these "cold traps" may harbor ice that has accumulated
over thousands of years (or even longer).

Dawn has peered into craters that might be cold traps. Of course, sunlight
doesn't illuminate them directly. But faint reflections from other parts
of the crater may be just barely bright enough that with long exposures
and special care in analyzing the pictures, new insights might come to

Dawn could continue operating in this orbit, but it has already squeezed
nearly as much out of its suite of sophisticated sensors as it can, and
it soon would reach the point of diminishing returns. In addition, its
lifetime here is now very limited. Although the hydrazine has lasted longer
than expected, the gauge on the tank is dropping relentlessly as the robotic
ship uses the propellant to counter the strong gravitational torque at
this low altitude. Even if the two functioning reaction wheels continue
to run correctly in hybrid control, the hydrazine would be exhausted early
next year, and the mission would come to an immediate end. And given the
premature death of the other two wheels, Dawn might not last even that
long. If one more wheel fails, Dawn's remaining lifetime would be cut
in half. At this point, how can we get the most out of Earth's deep-space
Dawn LAMO Image 135

Dawn observed this tortuous landscape at 70 degrees north latitude on
Feb. 4, 2016, from its current mapping orbit at an altitude of 240 miles
(385 kilometers). The impact that formed the lower crater partially obliterated
the older one above. As in the previous picture, sunlight comes from the
right. Look carefully, especially in the newer crater, to see large boulders,
which are bright on the right, as described in more detail here. You can
also see streaks of bright material on the crater wall. Full image and
caption. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

We have explained before that Dawn will never go closer to Ceres. There
are several reasons. The rate at which hydrazine is consumed depends quite
strongly on the altitude, so if the probe ventured lower, its lifetime
would be significantly shorter. (Similarly, at higher altitude, it uses
less hydrazine and so its lifetime would be longer.) Ceres has water (albeit
mostly frozen, although perhaps some as liquid), energy (both from the
distant sun and from radioactive elements incorporated when Ceres formed
more than 4.5 billion years ago), and some of the other important ingredients
for the development of life. We want to protect this astrobiologically
interesting environment from the spacecraft's terrestrial contamination,
so we cannot risk going low enough that it might crash, even long after
the mission concludes. (And a controlled landing is not possible.) Also,
at lower altitudes Dawn would orbit so fast that pictures and other measurements
would be smeared, reducing the benefit of being closer. There are other
reasons as well, but the bottom line is that this orbit is where Dawn
draws its bottom line.

Ever creative, the team has found new ways to increase the mission's scientific
productivity. Once again, the strategy involves changes never anticipated
and that may be contrary to what your intuition would suggest. For more
than two years, your correspondent has been emphasizing that this would
be Dawn's final orbit. Now, on Sept. 2, Dawn will begin flying to a higher

The prospect of raising the orbit also raises several natural questions
about what will happen in the coming months, including how, why and what
kind of cake will be served at the team's celebration on Sept. 27 of the
ninth anniversary of Dawn's launch. This month, let's look at how, and
as the team refines its plans for the other key questions, we will discuss
the answers in future Dawn Journals.

To gain altitude, Dawn will take advantage of its remarkable ion propulsion
system. Ion propulsion has enabled many bold missions from Star Trek to
Star Wars to NASA's unique expedition to orbit Vesta and Ceres, which
would have been not simply difficult but impossible with conventional
propulsion. And like the spaceships that in science fiction fly wherever
they want to go, now Dawn will use its xenon ions to maneuver to an orbit
it would not otherwise to able to reach. (Despite the similarity, there
are some ways in which Dawn differs from the fictional ships: our craft
uncompromisingly obeys all the laws of physics and carries relatively
few systems designed to destroy other ships in battle.)
Dawn LAMO Image 149

Dawn took this photo of peaks in the center of Dantu Crater on June 3,
2016, while orbiting at 240 miles (385 kilometers). We have seen other
intriguing parts of this 78-mile (126-kilometer) crater before, both from
this distance and from farther away (showing the entire crater). Full
image and caption. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

To climb higher, Dawn will essentially reverse the spiral route it took
down to its current orbit, much as it did when it ascended from Vesta.
(There are some interesting technical differences in the nature of this
trajectory from all of the other spirals. The design incorporates clever
new ideas from Dawn's celestial navigators. But to the casual interplanetary
observer, it will appear the same.) As with all of Dawn's activities,
you can follow its progress upward with the mission status updates.

After five weeks of ion thrusting, looping higher and higher, the spacecraft
will stop at about 910 miles (1,460 kilometers). Readers with eidetic
memories (or who reread past Dawn Journals) may note that that is very
close to the altitude of the third mapping orbit. However, the orientation
of the orbit will be different. The spaceship will still circle in a polar
orbit. It will travel over the north pole, then fly south above the face
of Ceres lit by the sun. After it passes over the south pole, it will
streak to the north over terrain hidden in the dark of night. But the
plane of this orbit will be rotated from that of the third mapping orbit.
The angle to the sun will be smaller, so Dawn will pass over a different
part of the sunlit hemisphere, gaining new perspectives on the extraterrestrial

At its current low altitude, Dawn is now completing a truly extraordinary
phase of its exploration of Ceres. But there is still much more to come,
with new scientific investigations, new discoveries and new adventures
at higher altitudes. Now that we have seen a little of the how, be sure
to look for upcoming Dawn Journals to learn more about the why (and about
the anniversary cake).

Dawn is 240 miles (385 kilometers) from Ceres. It is also 2.24 AU (208
million miles, or 335 million kilometers) from Earth, or 855 times as
far as the moon and 2.22 times as far as the sun today. Radio signals,
traveling at the universal limit of the speed of light, take 37 minutes
to make the round trip.
Received on Wed 21 Sep 2016 07:04:20 PM PDT

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