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THE ROSETTA PROGRAM

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(1)

THE ROSETTA

PROGRAM

D.Moura (CNES)

Content

The foundations

Some general aspects

Engineering

Development

Launch campaign

In flight operations

(2)

The foundations

The case for comets

• They very likely constitute the fossils bricks of the solar system

• They may have contributed to the life emergence on the Earth

(3)

Solar system formation

Link with life

Besides contributing to the formation of the Solar System, comets also appear to have played a key role in the evolution of life on Earth. Some theories suggest that they may have seeded our planet with a large portion of the organic material constituting the basic building blocks of life.

Observations show that comets are partly

composed of water and of complex carbon

molecules, the essential building blocks of life.

Today, it is generally accepted that planets and

comets have the same origin. Thus, information

collected on the comet composition and

evolution processes will allow us to reach

conclusions on the formation and early evolution

(4)

Historical case of comets

Comets have been observed and recorded in China since the Shang Dynasty (1600/1046 BC).

The set of comet illustrations shown here is from a silk book written during the Han period (206/220 BC) . The different shapes and characteristics of the comet tails were outlined and on some of the comets, differences in the appearance of the core of the comet were noted.

(5)

Besides contributing to the formation of the Solar System, comets also appear to have played a key role in the evolution of life on Earth. Some theories suggest that they may have seeded our planet with a large portion of the organic material constituting the basic building blocks of life.

Historical case of comets

What is a comet ?

With space missions, we have a few images of comet nucleus:

• Halley (1986, Giotto)

• Borrelly (2001, Deep Space 1)

• Wild2 (2004, Stardust)

• Tempel1 (2005, Deep Impact)

(6)

What is a comet ?

They appear to be very fragile bodies where outgassing processes may be particularly violent

Model of the nucleus of the Halley comet

Why do they have tails ?

As a comet approaches the Sun,

outgassing leads to the formation

of a dust cloud called the coma,

which may trail a long distance

behind the comet in the form of a

tail blown by solar radiation

pressure and drawn out by the

solar wind.

Most known comets follow a highly elliptical trajectory bringing them periodically close to the Sun.

(7)

Some general aspects

Rosetta scientific objectives & measurements

Prime objective: comet observation:

• Origin of comets

• Role in the solar system formation

• Relationship with interstellar material

• Potential link with life

Scientific measurements to be performed to meet these objectives:

• Global characterization of the nucleus

• Characterization of the volatile and refractory materials

(8)

Why these names ?

A project has to have a name easy to remember and attractive, including for public

Programmatic aspects

Rosetta development has followed the classical phasing A, B, C/D and E. However, due its

complexity and the launcher problem, the overall duration up to the launch has been long (8 years).

Overall budget ~ 1 G €

(9)

Engineering

Engineering: the theoretical case

MISSION REQUIREMENTS

ORBIT(S) PAYLOAD

LAUNCHER

COST but ...

(10)

Engineering: the real case

OK : implement development Yes MISSION REQUIREMENTS ORBIT(S) PAYLOAD SPACECRAFT(S) LAUNCHER COST OBJECTIVE No GROUND SEGMENT Fits ? INTERNATIONAL COOPERATION RE-ASSESS EVERYTHING (and change timescale)

and/or

(11)

The Rosetta trajectory

CD Lander

The Rosetta orbiter

(12)

Descent Parameters

duration: beween 0.5 and 3 h impulse < 1 m/s

Landing Parameters

impact velocity : < 1.2 m/s impact angle: < 30 deg attack angle: < 30 deg

Initial Orbit

altitude > 1 km

no éclipse, no impact, no escape

Separation Parameters

amplitude dV < 0.53 m/s (in flight tunable) accuracy dV: 1 %, 0.3 deg (1 sigma)

V comet Landing relative velocity V lander at landing

Impulse at landing and harpoons firing

V orbiter V lander after separation

Impulse during descent (if needed)

dV separation

The Philae lander trajectory

The Philae lander

(13)

The ground segment

New Norcia & Camberra stations

(14)

The Mechanical & Structural models

Used to validate (at qualification levels) the mechanical and thermal architectures and to generate the final mechanical and thermal specifications of all units

The Electrical models

(15)

The Flight models

Used for verification and control (proto-fligth levels)

Launch campaign

(16)

The launch campaign : arrival in Rochambeau airport

(17)

The launch campaign:

deployment tests

The launch campaign: Electrical test and setting

(18)

The launch campaign: satellite fuelling

(19)

Launch

Rosetta successfully lifted off from Europe's Spaceport in Kourou, French Guiana, at 04:17 local time (08:17 CET) on 2 March 2004

(20)

The inflight operations : commissioning

Immediatly after the launcher separation the spacecraft is activated autonomatically and progressively, through TM/TC links it gets its final configuration. Then the inflight tests are

performed during several weeks to check all the equipments & sub-systems

Satellite solar arrays viewed from the c-lander’s camera CIVA

(21)

The inflight operations : Mars swing-by

The inflight operations : asteroids swing-bys

Asteroid Lutetia (July 2010) Asteroid Steins

(22)

Conclusions

And to finish …

A HUMAN CHALLENGE BETWEEN INDIVIDUALS !

A HUMAN CHALLENGE BETWEEN INDIVIDUALS !

A project is of course a technical challenge, but it is also…

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Advancement of non - involved Chaos

Panic

Search for the guilty

Punishment of the innocent Disillusion Wild Enthusiasm T H E R E A L P H A S E S O F A S P A C E P R O J E C T

Thanks for your attention

Questions ?

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