1. 2. 3. You have decided to join the ranks of Absurdly Rich Space Tourists (ARST) and go on a wonderful vacation to Mars and back. That should make all the other ARST insanely jealous since you are going to Mars and they never even got into Earth orbit. For the orbital dynamics part of your vacation planning assume that Earth is in a circular orbit 1.00 AU from the Sun, Mars is in a circular orbit 1.52 AU from the the Sun, and that the the orbits are coplanar. The orbit you plan to use for your trip is an ellipse with the Sun at one focus (Kepler's 1st Law). The perihelion of the ellipse is at Earth's orbit at 1.00 AU and the aphelion is at Mars' orbit at 1.52 AU. Your spacecraft will go around the Sun in the same sense as Earth and Mars. The orbit you have chosen for your trip is called a Hohmann Transfer Orbit. For this problem assume that the orbital period of Earth is 365 days and the orbital period of Mars is 684 days. Check that Kepler's Third Law holds for Earth and Mars. What is the semi-major axis a of the spacecraft's orbit? What is the eccentricity e of the spacecraft's orbit? What is the orbital period of the spacecraft? How long does it take to get to Mars? How long does it take to get from Mars to Earth?
1. 2. 3. You have decided to join the ranks of Absurdly Rich Space Tourists (ARST) and go on a wonderful vacation to Mars and back. That should make all the other ARST insanely jealous since you are going to Mars and they never even got into Earth orbit. For the orbital dynamics part of your vacation planning assume that Earth is in a circular orbit 1.00 AU from the Sun, Mars is in a circular orbit 1.52 AU from the the Sun, and that the the orbits are coplanar. The orbit you plan to use for your trip is an ellipse with the Sun at one focus (Kepler's 1st Law). The perihelion of the ellipse is at Earth's orbit at 1.00 AU and the aphelion is at Mars' orbit at 1.52 AU. Your spacecraft will go around the Sun in the same sense as Earth and Mars. The orbit you have chosen for your trip is called a Hohmann Transfer Orbit. For this problem assume that the orbital period of Earth is 365 days and the orbital period of Mars is 684 days. Check that Kepler's Third Law holds for Earth and Mars. What is the semi-major axis a of the spacecraft's orbit? What is the eccentricity e of the spacecraft's orbit? What is the orbital period of the spacecraft? How long does it take to get to Mars? How long does it take to get from Mars to Earth?
Related questions
Question
Astronomy
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SPACEFLIGHT - A TRIP TO MARS AND BACK
You have decided to join the ranks of Absurdly Rich Space Tourists (ARST) and
go on a wonderful vacation to Mars and back. That should make all the other ARST
insanely jealous since you are going to Mars and they never even got into Earth orbit.
For the orbital dynamics part of your vacation planning assume that Earth is
in a circular orbit 1.00 AU from the Sun, Mars is in a circular orbit 1.52 AU from the
the Sun, and that the the orbits are coplanar. The orbit you plan to use for your trip
is an ellipse with the Sun at one focus (Kepler's 1st Law). The perihelion of the ellipse
is at Earth's orbit at 1.00 AU and the aphelion is at Mars' orbit at 1.52 AU. Your
spacecraft will go around the Sun in the same sense as Earth and Mars. The orbit
you have chosen for your trip is called a Hohmann Transfer Orbit.
For this problem assume that the orbital period of Earth is 365 days and the
orbital period of Mars is 684 days.
Check that Kepler's Third Law holds for Earth and Mars.
What is the semi-major axis a of the spacecraft's orbit? What is the eccentricity e
of the spacecraft's orbit?
What is the orbital period of the spacecraft? How long does it take to get to Mars?
How long does it take to get from Mars to Earth?
When (at what Earth - Mars configuration) do you launch to go? In other words, where
does Mars need to be relative to Earth in order for you to get to Mars successfully?
Where is Earth when you arrive at Mars?
Where does Earth need to be relative to Mars for you to return safely to Earth?
How long to you have to wait on Mars before you can launch for home?
What is your total trip time? Care to go?
If you miss your launch configuration in question 4 or 6/7, how long do you
have to wait for the next one?"
Transcribed Image Text:1.
2.
3.
4.
5.
6.
7.
8.
9.
SPACEFLIGHT - A TRIP TO MARS AND BACK
You have decided to join the ranks of Absurdly Rich Space Tourists (ARST) and
go on a wonderful vacation to Mars and back. That should make all the other ARST
insanely jealous since you are going to Mars and they never even got into Earth orbit.
For the orbital dynamics part of your vacation planning assume that Earth is
in a circular orbit 1.00 AU from the Sun, Mars is in a circular orbit 1.52 AU from the
the Sun, and that the the orbits are coplanar. The orbit you plan to use for your trip
is an ellipse with the Sun at one focus (Kepler's 1st Law). The perihelion of the ellipse
is at Earth's orbit at 1.00 AU and the aphelion is at Mars' orbit at 1.52 AU. Your
spacecraft will go around the Sun in the same sense as Earth and Mars. The orbit
you have chosen for your trip is called a Hohmann Transfer Orbit.
For this problem assume that the orbital period of Earth is 365 days and the
orbital period of Mars is 684 days.
Check that Kepler's Third Law holds for Earth and Mars.
What is the semi-major axis a of the spacecraft's orbit? What is the eccentricity e
of the spacecraft's orbit?
What is the orbital period of the spacecraft? How long does it take to get to Mars?
How long does it take to get from Mars to Earth?
When (at what Earth - Mars configuration) do you launch to go? In other words, where
does Mars need to be relative to Earth in order for you to get to Mars successfully?
Where is Earth when you arrive at Mars?
Where does Earth need to be relative to Mars for you to return safely to Earth?
How long to you have to wait on Mars before you can launch for home?
What is your total trip time? Care to go?
If you miss your launch configuration in question 4 or 6/7, how long do you
have to wait for the next one?

Transcribed Image Text:Orbit
of Mors
Orbit
of Earth
Earth
at Departure
Kepler's Thir 2 Law.
3
(9)
Az
a₁
Perihelion:
Aphelion:
Гр
A =
Sun
a = {(₁ + r)
e =
PA-re
PA+rp
a(1-e)
a(lte)
Mars at Arrival
Kepler's Second Law - Circular Onkit
88= 360° ( 4 )
At: Elapsed Time
so= Angle Orbited Through
P = Orbital Period
Closest to Sun
Farthest from Sun
Spacecraft
Orbit
Semi-Major Axis
Eccentricity
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