Dawn (spacecraft)

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Dawn
Artist's concept of Dawn with Vesta (left) & Ceres (right) (the proximity of Vesta to Ceres is artistic license)
Organization	NASA
Major contractors	Orbital Sciences, JPL, UCLA
Mission type	Flyby/Orbiter
Satellite of	Mars (flyby) Vesta then Ceres
Launch date	September 27, 2007, 7:34 a.m EDT (11:34 UTC)[1]
Launch vehicle	Delta 7925H
Mission duration	8 years
NSSDC ID	DAWN
Webpage	Dawn Home
Mass	1,250 kg (2,756 lb)
Orbital elements
Eccentricity	~ circular
Inclination	Polar

Dawn, launched on September 27, 2007, is a robotic spacecraft being sent by NASA on a space exploration mission to the two most massive members of the asteroid belt: the asteroid Vesta and the dwarf planet Ceres. Dawn is scheduled to explore Vesta between 2011 and 2012, and Ceres in 2015. It will be the first spacecraft to visit either body.

Dawn is innovative in that it will be the first spacecraft to enter into orbit around a celestial body, study it, and then re-embark under powered flight to proceed to a second target. All previous multi-target study missions—such as the Voyager program—have involved rapid planetary flybys.

Contents 1 Launch 2 Mission 2.1 Mission team 3 Motivation 4 Mission cancellations and reinstatements 5 Propulsion system 6 The Dawn microchip 7 References and notes 8 See also 9 External links

[edit] Launch

Dawn was scheduled to launch from pad 17-B at the Cape Canaveral Air Force Station on a Delta 7925-H rocket.^[2] On April 10, 2007, Dawn arrived at the Astrotech Space Operations subsidiary of SPACEHAB, Inc. in Titusville, Florida, where it was prepared for launch.^[3][4] Launch was originally scheduled for 20 June, but was delayed until 30 June due to delays with part deliveries.^[5] A broken crane at the launch pad, used to raise the solid rocket boosters, delayed the launch for a week, until 7 July, but on June 15 the second stage was successfully hoisted into position.^[6][7] A mishap at the Astrotech Space Operations facility, involving slight damage to one of the solar arrays, did not have an effect on the launch date, however bad weather caused the launch to slip to 8 July. Range tracking problems then delayed the launch to 9 July, and then 15 July, before the launch was delayed further to avoid knock-on delays with the Phoenix mission to Mars, which was successfully launched on 4 August.

Launch of Dawn was then rescheduled for September 26, 2007.^[8][9] However the launch was then delayed to 27 September, due to bad weather delaying fuelling of the second stage, the same problem which had earlier delayed the 7 July launch attempt. The launch window extended from 7:20 a.m. - 7:49 a.m. EDT (11:20 - 11:49 GMT).^[10] During the final built-in hold at T-4 minutes, a ship entered the exclusion area offshore, the sea strip where the rocket boosters are likely to fall after separation. The ship was commanded to leave the area, then the launch had to wait for the end of a collision avoidance window with the ISS.^[11] The spacecraft finally launched at 7:34 a.m. EDT from pad 17-B on a Delta II launch vehicle.^[12][13][14]

[edit] Mission

The mission's goal is to characterise the conditions and processes of the solar system's earliest epoch by investigating in detail two of the largest protoplanets remaining intact since their formation. Ceres and Vesta have many contrasting characteristics that are thought to have resulted from them forming in two different regions of the early solar system; Ceres is theorized to have experienced a "cool and wet" formation that may have left it with subsurface water, and Vesta is theorised to have experienced a "hot and dry" formation that resulted in a differentiated interior and surface volcanism.

Using a framing camera along with two redundant cameras,^[15] a visual and infared spectrometer, and a Gamma Ray and Neutron Spectrometer,^[16] Dawn will take pictures and measure the chemical composition of Ceres and Vesta.^[17]

To cruise from Earth to its targets it will travel in a long outward spiral. The current estimated chronology is as follows:^[18]

• September 27, 2007: launch
• February 2009: Mars gravity assist
• September 2011: Vesta arrival
• April 2012: Vesta departure
• February 2015: Ceres arrival
• July 2015: End of operations

An extended mission in which Dawn explores other asteroids after Ceres is also possible, although unlikely.^{[citation needed]}

[edit] Mission team

The Dawn mission team is led by UCLA space scientist and Dawn Principal Investigator Christopher T. Russell. Michael Mook is the Dawn Program Manager at Orbital Sciences Corporation, which built the spacecraft. Armando Piloto is the Dawn Mission Manager at Kennedy Space Center. NASA's Jet Propulsion Laboratory provided the Ion Propulsion System and management of the overall flight system development. The German Aerospace Center (DLR) and the Max Planck Institute for Solar System Research provided the framing camera, the Italian Space Agency provided the mapping spectrometer, and the DOE Los Alamos National Laboratory provided the gamma ray and neutron spectrometer.^[19]

[edit] Motivation

Dawn is intended to study two large asteroids in order to answer questions about the formation of the solar system.

Ceres and Vesta were chosen as two contrasting protoplanets, one apparently "wet" (that is, icy) and the other "dry" (or rocky), whose accretion was terminated by the formation of Jupiter. They provide a bridge in our understanding between the formation of rocky planets and the icy bodies of our solar system, and under what conditions a rocky planet can hold water.

The IAU adopted a new definition of planet on August 24, 2006, and thus, if the IAU's definition stands and the spacecraft experiences no delays, Dawn will become the first mission to study a dwarf planet, arriving at Ceres five months prior to the arrival of New Horizons at Pluto.

Ceres is a dwarf planet whose mass encompasses about one-third of the total mass of the asteroids in the asteroid belt and whose spectral characteristics suggest a composition similar to that of a water-rich carbonaceous chondrite. Smaller Vesta, a water-poor achondrite, has experienced significant heating and differentiation. It shows signs of a metallic core, a Mars-like density and lunar-like basaltic flows.

Both bodies formed very early in the history of the solar system, thereby retaining a record of events and processes from the time of the formation of the terrestrial planets. Radionuclide dating of pieces of meteorites thought to come from Vesta suggests that Vesta differentiated quickly, in only three million years. Thermal evolution studies suggest that Ceres must have formed a little later, more than three million years after the formation of CAIs (the oldest known objects of Solar System origin).

Moreover, Vesta is the source of many smaller objects in the solar system. Most (but not all) V-type near-Earth asteroids, and some outer main-belt asteroids have spectra similar to Vesta and are known as 'vestoids'. Five percent of the found meteoritic samples on Earth, the Howardite Eucrite Diogenite ("HED") meteorites, are thought to be the result of a collision or collisions with Vesta.

[edit] Mission cancellations and reinstatements

The status of the Dawn mission has changed several times. In December, 2003, the project was first cancelled,^[20] and then reinstated in February, 2004. In October, 2005, work on Dawn was placed into "stand down" mode. In January, 2006, Dawn's "stand down" was discussed in the press as "indefinitely postponed", even though NASA had announced no new decisions regarding the mission's status.^[21] On March 2, 2006, Dawn was publicly, but not formally cancelled by NASA headquarters.^[22]

In an unusual step, the cancellation was placed under review,^[23] and on 27 March 2006, it was announced that the mission would not be cancelled after all.^[24][25] In the last week of September 2006, the Dawn mission instrument payload integration reached a full functional status.

[edit] Propulsion system

The Dawn spacecraft is propelled by three DS1 heritage xenon ion thrusters (firing only one at a time). They have a specific impulse of 3100 s and produce a thrust of 90 mN.^[26] The whole spacecraft, including the ion propulsion thrusters, is powered by a 10 kW triple-junction solar array.^[27] To get to Vesta, Dawn will use 275 kg (606 lb) Xe and another 110 kg (243 lb) to get to Ceres,^[28] out of a total of 425 kg (937 pounds) of on-board propellant.^[29] All in all, it will perform a velocity change of over 10 km/s, far more than any other spacecraft has done.^[28] Dawn is NASA’s first purely exploratory mission to use ion propulsion engines.^[30]

After initial checkout, during which the ion thrusters accumulated more than 11 days of thrust, Dawn began long-term cruise propulsion on 2007-12-17.^[31]

[edit] The Dawn microchip

Onboard Dawn is a small computer microchip bearing the names of more than 360,000 space enthusiasts.^[32] The names were submitted online as part of a public outreach effort between September 2005 and November 4, 2006.^[33] The microchip (about the size of a nickel) was installed above the forward ion thruster, underneath the spacecraft's High Gain Antenna, on May 17, 2007.^[34] More than one microchip was made, with a back-up copy on display at the 2007 Open House at the Jet Propulsion Laboratory in Pasadena, California.

[edit] References and notes

[edit] See also

• Delta II
• Ceres (dwarf planet)
• 4 Vesta
• 2007 in spaceflight

[edit] External links

• The Wikimedia Commons has media related to Dawn (spacecraft).
• Where is Dawn Now - from JPL, images updated regularly
• Dawn mission home page at JPL
• Dawn mission home page at NASA
• Dawn Website at UCLA Space Physics Center
• Dawn Mission Profile by NASA's Solar System Exploration
• Visual and Infrared Spectrometer Instrument at INAF (Istituto Nazionale di Astrofisica)
• Dawn Framing Camera at Max Planck Institute for Solar System Research
• Gamma Ray and Neutron Spectrometer for Dawn, short paper on the instrument, from 37th Lunar and Planetary Science Conference
• Dawn news coverage.

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