[meteorite-list] Dawn Journal

From: info at moonmarsrocks.com <info_at_meteoritecentral.com>
Date: Thu, 06 Sep 2012 10:45:35 -0700
Message-ID: <20120906104535.b86ea499b59be1b7298b47d2f1127a77.074a391733.wbe_at_email13.secureserver.net>

Thanks, Ron, for sharing Dr.Rayman's eloquent journal log.
Looking forward to Dawn's next adventure at Ceres, including spectral
analysis that might shed light on whether there are Ceres-derived
meteorites here on Earth.
 
Best,
Daniel

Daniel Noyes
www.moonmarsrocks.com

 
  
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Message: 11
Date: Wed, 5 Sep 2012 15:14:01 -0700 (PDT)
From: Ron Baalke <baalke at zagami.jpl.nasa.gov>
Subject: [meteorite-list] Dawn Journal - September 5, 2012
To: meteorite-list at meteoritecentral.com (Meteorite Mailing List)
Message-ID: <201209052214.q85ME1Jk024956 at zagami.jpl.nasa.gov>
Content-Type: text/plain; charset=us-ascii


http://dawn.jpl.nasa.gov/mission/journal_09_05_12.asp

Dawn Journal
Dr. Marc Rayman
September 5, 2012

Dear Marvestalous Readers,

An interplanetary spaceship left Earth in 2007. Propelling itself
gently and patiently through the solar system with a blue-green
beam of xenon ions, it gradually spiraled away from the sun. It sailed
past Mars in 2009, its sights set on more distant and exotic
destinations. In July 2011, it gracefully and elegantly entered orbit
around the second most massive resident of the main asteroid belt,
Vesta. It spent more than 13 months there scrutinizing the gigantic
protoplanet with all of its sensors and maneuvering to different orbits
to optimize its investigations, making myriad marvelous discoveries.
After they traveled together around the sun for 685 million kilometers
(426 million miles), the ship left orbit in September 2012 and is now
headed for dwarf planet Ceres, the largest body between the sun and
Neptune not yet visited by a spacecraft. No other probe has ever been
capable of the amazing feats Dawn is performing, exploring two of the
largest uncharted worlds in the inner solar system.

The population of the main asteroid belt numbers in the millions. Vesta
is such a behemoth that Dawn has now single-handedly examined about
eight percent of the mass of the entire belt. And by the time it
finishes
at the colossus Ceres, it will have investigated around 40 percent.

The expedition to Vesta has produced riches beyond everyone's hopes.
With 31,000 photos, 20 million visible and infrared spectra, and
thousands
of hours of neutron spectra, gamma ray spectra, and gravity
measurements,
Dawn has revealed to humankind a unique and fascinating member of the
solar system family. More akin to Earth and the other terrestrial
planets
than to typical asteroids, Vesta is not just another chunk of rock. It
displays complex geology and even has a dense iron-nickel core, a
mantle,
and a crust. Its heavily cratered northern hemisphere tells the story of

more than 4.5 billion years of battering in the rough and tumble
asteroid
belt. Its southern hemisphere was wiped clean, resurfaced by an enormous

impact at least two billion years ago and an even greater collision one
billion years ago. These events excavated the 400-kilometer (250-mile)
Veneneia and 500-kilometer (310-mile) Rheasilvia basins. The larger
basin
has a mountain at the center that towers more than twice the height of
Mt. Everest; indeed, it soars higher than all but one of the mountains
known in the solar system. The impacts were so forceful, they nearly
destroyed Vesta. The fierce shock reverberated through the entire body
and left as scars an extraordinary network of vast troughs near the
equator, some hundreds of kilometers (miles) long and 15 kilometers
(10 miles) wide.

The powerful impacts liberated tremendous amounts of material, flinging
rocks far out into space, some of which eventually made it all the way
to Earth. It is astonishing that about six percent of the meteorites
found here came from Vesta. We have some meteorites from Mars, and we
have some meteorites from the moon, but we have far, far more that
originated in those impacts at Vesta, so distant in time and space.
Vesta, Mars, and the moon are the only celestial bodies identified as
the source of specific meteorites.

Scientists will spend years productively poring through Dawn's fabulous
findings and learning what secrets they hold about the dawn of the solar
system, and many more people will continue to marvel at the spectacular
sights of this alien world. But the emissary from Earth has completed
its assignment there and moved on. It has spent most of its time since
the previous log using its ion propulsion system to climb higher and
higher above Vesta. This departure spiral is the mirror image of the
approach spiral the robotic adventurer followed last year. The unique
method of entering and leaving orbit is one of the many intriguing
characteristics of a mission that uses ion propulsion. Without that
advanced technology, this ambitious deep space adventure would be
impossible.

As Dawn ascended, Vesta's gravitational grip grew weaker and weaker. At
some point along its spiral, the explorer was far enough and moving fast
enough that Vesta could no longer hold it in orbit. As smoothly and
tenderly as Vesta had taken Dawn in its embrace last year,
it released its erstwhile companion, each to go
its own way around the sun. The bond was severed at about 11:26 p.m. PDT
yesterday, when they were 17,200 kilometers (10,700 miles) apart,
separating at the remarkably leisurely speed of less than 33 meters per
second (73 miles per hour). Many of our readers drove their cars that
fast today (although we hope it was not in school zones).

Unlike missions that use conventional chemical propulsion, there was no
sudden change on the spacecraft and no nail-biting on Earth. If you had
been in space watching the action, you probably would have been hungry,
cold, and hypoxic, but you would not have noticed anything unusual about
the scene. Apart from a possible hint of self-satisfaction, Dawn would
have looked just as it had for most of its interplanetary flight, a
monument to humankind's ingenuity and passionate drive to know the
cosmos perched atop a blue-green pillar of xenon ions. If, instead, you
had been in Dawn mission control watching the action, you would have
been in the dark and all alone (until JPL Security arrived). There was
no need to have radio contact with the reliable spaceship. It had
already thrust for almost 2.9 years, or 58 percent of its time in space.
Thrusting during escape was no different. No one was tense or anxious;
rather, all the drama is in the spectacular results of the bold mission
at Vesta and the promise of what is to come at Ceres. When Dawn entered
orbit, your correspondent was dancing. When Dawn left orbit, he was
sleeping serenely [Webmaster: please link "sleeping serenely" to the
site containing the detailed records of my dreams].

A month earlier, on August 8, with the craft more than 2,100 kilometers
(1,300 miles) above the surface, patiently powering its way up through
Vesta's gravity field, one of the reaction wheels experienced an
increase in internal friction. Reaction wheels are used to control a
spacecraft's orientation in the frictionless, zero-gravity conditions of
spaceflight. By electrically changing a wheel's spin rate, Dawn can
rotate or stabilize itself. Protective software quickly detected the
event and correctly responded by deactivating that wheel and the other
two that were operating, switching to the small jets that are available
for the same function, and reconfiguring other systems, including
powering off the ion thrust and turning to point the main antenna to
Earth.

A routine communications session the next day revealed to mission
controllers what had occurred. They had planned long ago
to turn the wheels off for the flight
from Vesta to Ceres, so having them off a few weeks early was not a
significant change. The team soon restored the spacecraft to normal
operations and reformulated the departure plan, and on August 17 Dawn
resumed its ascent. Because of the hiatus in thrusting, escape shifted
from August 26 to September 4. The flexibility in the mission timeline
provided by ion propulsion made this delay easy to accommodate.

In order to conserve the hydrazine propellant
that the jets use, the bonus departure observations described before
were curtailed, as they were not a high priority for the mission.
Nevertheless, on August 25 and 26, at an altitude of around 6,000
kilometers (3,700 miles), the explorer did peer at Vesta once more
with its camera and visible and infrared mapping. The last time it
had been this far away was July 21, 2011, during its descent to an
unfamiliar destination. This time, 13 months later, the spacecraft
turned back for a final gaze at the magnificent world it had unveiled
during its remarkable time there, a world that prior to last year had
appeared as little more than a tiny smudge among the stars for the two
centuries it had been observed.

The delay in the departure schedule provided a convenient benefit. Vesta
has seasons, just as Earth does, although they progress more slowly on
that distant orb. August 20 was the equinox, when northern hemisphere
spring began. Until then, the sun had been in Vesta's southern
hemisphere
throughout Dawn's residence there. While most of the northern hemisphere

was revealed during the second high-altitude mapping orbit, the
illumination
of the landscape immediately around the north pole was even better for
this
last look. After radioing its parting shots to wistful mission
controllers, the ship commenced its climb again.

And then, with an stunningly successful mission behind it, a newly
explored world below it, and a mysterious dwarf planet ahead of it, the
indomitable and indefatigable adventurer left Vesta forever.

Dawn is 18,500 kilometers (11,500 miles) from Vesta and 64 million
kilometers (40 million miles) from Ceres. It is also 2.45 AU (367
million kilometers or 228 million miles) from Earth, or 910 times as far
as the moon and 2.43 times as far as the sun today. Radio signals,
traveling at the universal limit of the speed of light, take 41 minutes
to make the round trip.


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Received on Thu 06 Sep 2012 01:45:35 PM PDT