Using Venus in the Parker Solar Probe mission

  • Context: High School 
  • Thread starter Thread starter sophiecentaur
  • Start date Start date
  • Tags Tags
    Probe Solar Venus
Click For Summary

Discussion Overview

The discussion centers on the use of gravity assist from Venus in the Parker Solar Probe mission, specifically how this maneuver will allow the probe to lower its orbit closer to the Sun over a series of flybys. Participants explore the mechanics of gravitational interactions and energy changes involved in this process.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants explain that the Parker Solar Probe will utilize gravity assists from Venus to decrease its orbital energy and approach the Sun over seven years.
  • One participant describes the mechanics of the gravity assist, suggesting that the probe must pass "on the other side" of Venus to slow down, akin to using retro rockets.
  • Another participant challenges the idea of energy loss, questioning how a change in direction without a change in kinetic energy can equate to the effect of retro rockets.
  • There is a discussion about the frame of reference, with one participant noting that while Venus's kinetic energy remains unchanged in its own frame, the relevant changes should be considered from the Sun's frame.

Areas of Agreement / Disagreement

Participants express differing views on the mechanics of the gravity assist and the implications for kinetic energy changes. There is no consensus on the interpretation of how the probe's orbit is altered through this maneuver.

Contextual Notes

Participants acknowledge the complexity of visualizing the gravitational interactions and the implications of frame of reference in understanding the energy changes involved.

sophiecentaur
Science Advisor
Homework Helper
Messages
30,403
Reaction score
7,470
The Parker Solar Probe mission will be launched soon and I was reading that it will use gravity assist from Venus to bring its orbit closer and closer to the Sun over about seven years.
The diagram in this link shows the plan for seven flyby's of Venus to lower the orbit. Now, to get down close to the Sun, the probe needs to lose potential energy so , unlike with space shots that take probes to outer planets, where the probes acquire Kinetic Energy on their flyby's, the probe's orbital energy needs to be reduced. So it looks like the probe needs to pass Venus 'on the other side' so that it accelerates Venus and slows down the probe, just as if it were using retro rockets.
Can someone confirm this or put me right on the details, please?
 
Astronomy news on Phys.org
I'm bumping this because it strikes me as a topic worth discussing - when you read so many comments about getting out of the Solar system using the same method.
I'm wondering about posting a similar question in General Physics.
 
sophiecentaur said:
The Parker Solar Probe mission will be launched soon and I was reading that it will use gravity assist from Venus to bring its orbit closer and closer to the Sun over about seven years.
The diagram in this link shows the plan for seven flyby's of Venus to lower the orbit. Now, to get down close to the Sun, the probe needs to lose potential energy so , unlike with space shots that take probes to outer planets, where the probes acquire Kinetic Energy on their flyby's, the probe's orbital energy needs to be reduced. So it looks like the probe needs to pass Venus 'on the other side' so that it accelerates Venus and slows down the probe, just as if it were using retro rockets.
Can someone confirm this or put me right on the details, please?

The figure is not helpful for your questions, but you are correct. In Venus's frame, the probe accelerates it slightly by passing "in front" of Venus on the probe's path to the inner Solar System and pulls it to a higher orbit. "In front" here means, in the direction of Venus's instantaneous orbital velocity -- let's say, for concreteness, that means between Venus and Antares at that moment.

Conversely, in the probe's frame, by passing between Venus and Antares (they agree on the geometry when expressed this way!), the probe experiences an acceleration that sends it more directly toward the Sun. Even though its asymptotic speed [that is, pre & post-encounter] relative to Venus does not change, it has given Venus some of its orbital energy and "falls" into a smaller orbit about the Sun.
 
JMz said:
it has given Venus some of its orbital energy and "falls" into a smaller orbit
I guess that's oneway of describing what goes on. But, if there is just a change of direction, with no loss of speed (KE), then where is the equivalent action of a retro rocket which is the more common way of dropping down an orbit?
The retro rocket method involves a (-KE) burst whilst at apogee to reduce orbital energy. Your interpretation implies a change in position, after passing by Venus. That's hard to visualise but I could be convinced, I suppose.
PS I take your point about the usefulness of the diagram but it's all I could get hold of.
 
@JMz I just re read your post and I had missed out the Frame of Venus bit. Its KE is not changed in that frame but are we not concerned by the KE change in the Sun's Frame?
I don't think this needs to be pursued much further as I am getting the idea now.
Cheers.
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 18 ·
Replies
18
Views
3K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 30 ·
2
Replies
30
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 23 ·
Replies
23
Views
10K
  • · Replies 1K ·
36
Replies
1K
Views
190K
  • · Replies 3 ·
Replies
3
Views
3K