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Voyager 2 was launched in 1977 to study the outer planets of the solar system. It utilized gravitational assists from Jupiter, Saturn, Uranus, and Neptune to alter its trajectory and reach these distant destinations. Voyager 2 made many discoveries about the atmospheres, magnetic fields, and moons of these planets. It continues its journey studying the heliopause and interstellar medium beyond the heliosphere.

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0% found this document useful (0 votes)
22 views3 pages

Real

Voyager 2 was launched in 1977 to study the outer planets of the solar system. It utilized gravitational assists from Jupiter, Saturn, Uranus, and Neptune to alter its trajectory and reach these distant destinations. Voyager 2 made many discoveries about the atmospheres, magnetic fields, and moons of these planets. It continues its journey studying the heliopause and interstellar medium beyond the heliosphere.

Uploaded by

gatherbouttech
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
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OBJECTIVE
To understand the physics behind the Voyager 2
satellite's journey through the outer solar system
and its scientific contributions to our
understanding of distant planets.

INTRODUCTION
Provide a brief overview of the Voyager 2
mission, including its launch date, purpose, and
the spacecraft's trajectory through the solar
system. Emphasize the importance of this
mission in advancing our knowledge of the outer
planets.
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PROJECT COMPONENTS
1. Trajectory Analysis:
● Gravity Assists: Voyager 2 utilized a gravitational slingshot effect
by flying by Jupiter, Saturn, Uranus, and Neptune in a specific
sequence. Each encounter provided a gravitational assist,
boosting the spacecraft's velocity and altering its trajectory.
● Physics Equations: The physics of gravitational assists involves
concepts like conservation of energy and angular momentum. You
can explore how these principles are applied in calculating the
trajectory changes.

2. Deep Space Communication:


● Communication Delays: Discuss the challenges of communicating
with a spacecraft that is billions of miles away. The physics of
signal travel time at the speed of light is crucial in understanding
communication delays.
● Antenna Systems: Explore the physics of the large dish antennas
on Earth that are used to communicate with Voyager 2. Discuss
the concept of signal strength and how it diminishes with
distance.

3. Instrumentation and Data Collection:


● Physics Instruments: Voyager 2 carried instruments such as
cameras, spectrometers, and magnetometers. Explain the physics
principles behind each instrument's operation and how they gather
data about the environment in space.
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● Data Transmission: Discuss the physics of data


transmission—how information is encoded, transmitted, and
decoded between the spacecraft and Earth.

4. Spacecraft Power and Thermal Systems:


● RTGs: Radioisotope thermoelectric generators (RTGs) convert the
heat produced by the decay of radioactive isotopes into electricity.
Explore the physics behind this process and how it sustained
power for Voyager 2 for decades.
● Thermal Regulation: Discuss the challenges of maintaining
optimal temperatures in space. How does the spacecraft manage
to dissipate excess heat and avoid freezing in the coldness of
outer space?

5. Discoveries and Contributions:


● Jupiter and Saturn Observations: Explore the physics of planetary
atmospheres, magnetospheres, and the interactions between
planetary rings and moons.
● Uranus and Neptune Exploration: Discuss the discoveries of these
ice giants, including their unique magnetic fields and atmospheric
compositions.

6. Interstellar Mission:
● Heliosphere and Heliopause: Explain the physics concepts related
to the heliosphere—the region influenced by the Sun's solar
wind—and the heliopause—the boundary where the solar wind
meets the interstellar medium.

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