Are the planets where we expect them to be

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Discussion Overview

The discussion revolves around the positioning of planets in relation to space probes, particularly addressing whether planets are where they are expected to be when probes arrive. The scope includes theoretical considerations, potential errors in modeling planetary positions, and the implications for space missions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant mentions a film suggesting that planets are not exactly where expected when space probes arrive, but does not understand the specifics of this claim.
  • Another participant argues that planets must be in their expected positions for probes to successfully arrive, suggesting that any discrepancies would be minimal and unlikely to cause mission failures.
  • A different participant proposes that course corrections made by probes are more likely due to errors in the probe's trajectory rather than inaccuracies in the planets' expected positions.
  • One participant discusses uncertainties in modeling planetary positions, noting a 1 km uncertainty for Mars over a span of 10-20 years, and highlights the complexities of probe navigation and measurement errors.
  • Several participants reference specific anomalies, such as the Pioneer anomaly and the flyby anomaly, questioning their relevance to the discussion about planetary positioning.
  • Another participant mentions the Yarkovsky effect and solar radiation pressure as factors that could impact spacecraft, but distinguishes these from the main concern of planetary positioning.

Areas of Agreement / Disagreement

Participants express differing views on the nature and significance of the discrepancies in planetary positioning. There is no consensus on the implications of these discrepancies or their relevance to the original claim from the film.

Contextual Notes

Participants note various sources of error in both planetary modeling and probe navigation, including uncertainties in ephemerides and measurement techniques. The discussion highlights the complexity of accurately predicting planetary positions over time.

Bjarne
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I saw a film some time ago at NGC.
It was told that the planets not are exactly there where expect them to be, when space probes arrives, but I did not got the point..
What is wrong ?
 
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Can you give the title of the film? I haven't heard of that problem, but I can tell you that the planets are there when probes arrive, otherwise the probes would miss, and we wouldn't have all the cool pictures we get from the probes on and around those planets.

But perhaps the film was talking about planets being just a tiny bit out of their expected position; maybe enough difference to be measured, but not enough to make the probe miss? That seems pretty unlikely, since the margine for error on interplanetary probe missions is very small. I'd like to search for the qoute from the film itself, if you can remember the title (and if it's in English).
 
LURCH said:
Can you give the title of the film? I haven't heard of that problem, but I can tell you that the planets are there when probes arrive, otherwise the probes would miss, and we wouldn't have all the cool pictures we get from the probes on and around those planets.

But perhaps the film was talking about planets being just a tiny bit out of their expected position; maybe enough difference to be measured, but not enough to make the probe miss? That seems pretty unlikely, since the margine for error on interplanetary probe missions is very small. I'd like to search for the qoute from the film itself, if you can remember the title (and if it's in English).

It's long ago
Yes it's only a tiny bit
 
More likely the course corrections the probes make are due to error in the probe's trajectory, not error in the expected position of the planet.
 
Bjarne said:
I saw a film some time ago at NGC.
It was told that the planets not are exactly there where expect them to be, when space probes arrives, but I did not got the point..
What is wrong ?

Since you cannot supply a source to determine what is truly being discussed, I suspect the problem is that the target planet is not where it is expected to be relative to the the incoming the space probe. Our imperfect modeling of the behavior solar system is a part of the total error. For example, there is about a 1 km uncertainty in Mars position over the last/next 10-20 years; errors increase moving forward or backward in time.

Additional error arises from not quite knowing the state of the probe. The probes navigate by dead reckoning, with occasional Kalman updates based on Deep Space Network measurements. DSN range rate measurements are incredibly precise (~ 1 mm/sec). Measurements of range, are also quite good (~ 1 m). Things get worse normal to line of sight. Cross range position error (observable by using multiple antenna) is on the order of a kilometer. Transverse velocity is not directly observable.

These are errors with respect to Earth -- and that brings us back to the uncertainties in the ephemerides.
 
twofish-quant said:
I suspect its more along the mundane lines alluded to above. The Pioneer anomaly is observable only in the tiny handful of vehicles that have gone well beyond the planets; the flyby anomaly is a tiny possibly unexplained change in velocity during a planetary flyby. Neither of these pertains to the "planet not being where we expect them to be."

Also just to give you an idea of the types of effects that do impact spacecraft , look at this http://en.wikipedia.org/wiki/Yarkovsky_effect
Force due to solar radiation pressure is much smaller than thrust uncertainty. It is an effect, but not much of one, during transit. (Note: This is not quite the same as the Yarkovsky effect. The Yarkovsky effect is a second order effect that results from tumbling. We do not like our spacecraft to be tumbling.) Torque due to solar radiation pressure does make for small but persistent perturbative effects during long term operations. For this reason, the Mars Reconnaissance Observer underwent am eight day solar radiation pressure calibration at the end of the cruise phase to Mars.
 

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