[meteorite-list] Dawn Journal - June 23, 2011

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Sun, 26 Jun 2011 18:56:23 -0700 (PDT)
Message-ID: <201106270156.p5R1uNZS024273_at_zagami.jpl.nasa.gov>

http://dawn.jpl.nasa.gov/mission/journal_06_23_11.asp

Dawn Journal
Dr. Marc Rayman
June 23, 2011

Dear Dawnstinations,

Vesta beckons, and Dawn responds. Now more than halfway through its
approach to Vesta, Dawn continues creeping up on the destination it
has been pursuing since it began its interplanetary travels. The
separation between them gradually shrinks as the probe's ion thrusting
brings its orbit around the sun into a closer and closer match with
Vesta's. At the same time, the giant protoplanet's gravity tugs gently
on the approaching ship, luring it into orbit.

Starting at the beginning of the approach phase on May 3, Dawn
interrupted thrusting once a week to photograph Vesta against the
background stars. These images help navigators determine exactly where
the probe is relative to its target. This technique does not replace
other means of navigation but rather supplements them. One of the
principal methods of establishing the spacecraft's trajectory relies
on accurately timing how long it takes radio signals, traveling, as
all readers know, at the universal limit of the speed of light, to make
the round trip between Earth and Dawn. Another uses the Doppler shift
of the radio waves, or the slight change in pitch caused by the craft's
motion. These sensitive measurements remain essential to navigating the
faraway ship as it sails the interplanetary seas.

Despite the very slow approach, the distance is small enough now that
observing Vesta weekly is no longer sufficient. To achieve the navigational
accuracy required to reach the intended orbit in early August, last week the
frequency of imaging was increased to twice per week. In each session,
half of the pictures are taken with long exposures to ensure many stars
are detectable, thus overexposing the much brighter disc of the nearby
Vesta. The other half use short exposures to ensure that the rocky world
shows up correctly so its precise location can be measured. The visible
and infrared mapping spectrometer has been commanded to observe Vesta
during three of these sessions, each time providing valuable information
that will help scientists select instrument settings for when Dawn is close
enough to begin its detailed scientific measurements.

In addition to the regular campaign of imaging for navigation, mission
controllers have other plans in store for the approach phase that were
laid out more than a year ago. Twice in the next few weeks, the spacecraft
will watch Vesta throughout its complete 5.3-hour rotation on its axis,
revealing exciting new perspectives on this uncharted body. The explorer
also will search for moons of the alien world.

There are several ways you can have the same spectacular views as Dawn
while it closes in on this immense protoplanet. You could build your own
ion-propelled interplanetary spaceship and travel to Vesta. Just imagine
how exciting that would be! But if you did that, the time to write all
the logs describing your adventure probably would make the
undertaking impractical. Another option would be to build your own
telescope. To see Vesta as clearly as Dawn sees it today, you would need
a telescope only three times the size of the Hubble Space Telescope.
Regrettably, then you would have to wait until Earth's and Vesta's
orbits around the sun brought them into closer alignment. In the
meantime, Dawn's camera would draw much closer to its subject. By the
beginning of August, it will see Vesta with more than 100 times the
clarity that Hubble could ever obtain. Still another alternative would
be to go here <http://dawn.jpl.nasa.gov/multimedia/vesta_dawn_gallery.asp>
to see some of the best views that humankind's robotic ambassador to the
asteroid belt has returned. New pictures will be added regularly.

A relic that bears witness to the dawn of the solar system, a colossus
that outweighs all other residents of the main asteroid belt save Ceres
(Dawn's second destination), a fuzzy point of light among the stars that
has intrigued and enticed astronomers for more than two centuries, a
mysterious orb that has stirred the passions of creatures on a distant
planet, inspiring them to dispatch an emissary to scrutinize it, is
finally being revealed as a unique and fascinating world. Dawn's images
delight and tantalize us, and the wait for still better views now is
brief indeed.

After more than 950 days of ion thrusting, with an effective change in
velocity of more than 6.6 kilometers per second (15,600 mph), Dawn's orbit
is so much like Vesta's that their paths around the sun are quite similar.
Less than a month ago, they were coming together at 240 meters
per second (540 mph). Today, the relative speed has declined to only 110
meters per second (250 mph). By July 16, Dawn will be traveling no
faster toward Vesta than you can drive in a car. The probe will be close
enough and slow enough that the protoplanet's gravity will tenderly take
the approaching explorer in its grasp. The next log will be posted
shortly after Dawn is in a high, loose orbit around Vesta, still
spiraling down toward survey orbit, where it will begin making detailed
studies of its home for the subsequent year.

Dawn is 152 thousand kilometers (95 thousand miles) from Vesta, or 40
percent of the average distance between Earth and the moon. It is also
1.39 AU (208 million kilometers or 129 million miles) from Earth, or 515
times as far as the moon and 1.37 times as far as the sun today. Radio
signals, traveling at the universal limit of the speed of light, take 23
minutes to make the round trip.
Received on Sun 26 Jun 2011 09:56:23 PM PDT