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Dawn - Explore the Cosmos | The Planetary Society
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Your 2012 Year in Space Calendar
  

Space Topics

Dawn


Dawn Journals: Dawn Project System Engineer Marc Rayman is contributing updates on the status of Dawn to The Planetary Society Weblog! Also, here's a summary of the Vesta phase of the mission.

Dec 30, 2011: The Om of orbit adjustment
Nov 29, 2011: Riding gravitational currents to LAMO
Oct 31, 2011: HAMO successfully completed, LAMO ahead
Sep 27, 2011: Fourth year in space, and arrival in HAMO
Sep 1, 2011: Spiraling down from Survey Orbit
Aug 11, 2011: In Survey Orbit
Jul 18, 2011: Dawn has arrived!!
Jun 23, 2011: Closing in on Vesta
May 27, 2011: Vesta to choose Dawn's arrival time
May 3, 2011: On the threshold of a new world
Mar. 31, 2011: Calibrating instruments and thrusters on Vesta approach
Feb. 27, 2011: HAMO2; the destination glows bright
Jan. 31, 2011: ORT ORT ORT
Dec. 30, 2010: LAMO (Low Altitude Mapping Orbit)
Nov. 30, 2010: Attitude Adjustment
Oct 31, 2010: Approaching conjunction
Sep 27, 2010: Third anniversary in space, and how to map Vesta
Aug 30, 2010: Getting warmer, farther from the Sun?
Jul 26, 2010: A Year from Vesta
Jun 27, 2010: Dawn 9.0
May 27, 2010: Surveying Vesta
Apr 28, 2010: Matching paces with Vesta
Mar 28, 2010: It's just a phase
Feb 28, 2010: Forever farther from Earth than the Sun
Jan 30, 2010: Thruster Two's time to shine
Dec 30, 2009: Patiently accelerating
Nov 27, 2009: In the asteroid belt, but far from asteroids
Oct 31, 2009: Taking up residence in the asteroid belt
Sep 27, 2009: Good performance means a longer stay at Vesta!
Aug 30, 2009: Earth catches up
Jul 31, 2009: Quiet Cruise
Jun 28, 2009: Back to powered flight
May 27, 2009: Testing Flight Software 8.0
Apr. 29, 2009: Upgrades!
Mar. 29, 2009: Safe without Safe Mode
Mar. 8, 2009: Safely past Mars
Feb. 13, 2009: Mars encounter
Jan. 27, 2009: Just missing the bull's eye at Mars
Dec. 30, 2008: Conjunction junction
Nov. 26, 2008: Aiming away from a bull's eye at Mars
Oct. 30, 2008: A pause in thrusting
Sep. 27, 2008: One year since launch
Aug. 28, 2008: Some explanations of orbital dynamics
Jul. 27, 2008: We crave power!
Jun. 26, 2008: Cruising past Mars' orbit
May 29, 2008: Dawn Journal
Apr. 22, 2008: Software updates
Mar. 30, 2008: One AUえーゆー from Earth
Mar. 3, 2008: Backup camera checks out
Jan. 31, 2008: Safely cruising
Dec. 17, 2007: Checkout complete, interplanetary cruise underway
Oct. 26, 2007: Testing, Testing, Testing
Nov. 14, 2007: Halfway through checkout
Oct. 9, 2007: Firing Up the Ion Propulsion System
Oct. 2, 2007: Launch!
Sep. 21, 2007: Awaiting launch II
September 14, 2007: What to expect after the launch II
September 5, 2007: Dawn prepares to launch II
Jul. 17, 2007: More than one way to leave the launch pad
Jul. 6, 2007: More bad weather - Awaiting launch
Jun. 26, 2007: What to expect after the launch
Jun. 12, 2007: Readying the rocket
Jun. 4, 2007: Dawn prepares for launch

Between the orbits of Mars and Jupiter circles the main asteroid belt, remnants of the formation of the solar system, millions of rocky bodies with orbits too disturbed by the gravitational pull of Jupiter for them to coalesce into a single planet. Among these are a few big ones, protoplanets that started down the road to terrestrial planethood but failed to thrive. Ceres and Vesta are the most massive of the minor planets, and the Dawn mission aims to visit them both to discover what clues they may hold to how our solar system, and particularly the terrestrial planets (Mercury, Venus, Earth, and Mars), formed.

Ceres and Vesta could hardly be more different. Ceres is a spherical, ice-rich world, similar (perhaps) to the icy moons of the outer solar system. Vesta is probably all rock and metal, and is so battered by past collisions with other asteroids that its shape is noticeably lumpy. Both bodies likely formed only 5 to 10 million years after the birth of the solar system, unlike Mars and Earth, which took much longer (30 and 50 million years, respectively). Although both formed in a relatively short period of time, Ceres was left with primordial water, while Vesta was not. The water at Ceres prevented it from developing the internal volcanic activity that developed on drier Vesta. Ceres' water almost certainly melted into a global subsurface ocean, and there may yet be liquid water beneath its icy crust.