Voyager 1: order-of-magnitude cross-track drift and speed loss over the next 100–1000 years

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SUMMARY

Voyager 1’s trajectory experiences an order-of-magnitude along-track lag of approximately 3.5 km after 100 years and about 350 km after 1000 years due to acceleration from interstellar neutral hydrogen and dust drag. The effective acceleration is calculated as 7×10⁻¹⁶ m/s² based on a velocity of 17 km/s, mass of 730 kg, cross-section of 10.75 m², and neutral hydrogen density of 0.1 cm⁻³ with a 1% dust-to-gas mass ratio. Cross-track deviations caused by gravitational perturbations and non-gravitational forces are negligible compared to the vast distance traveled (~500 billion km in 1000 years). These estimates rely on back-of-envelope calculations consistent with known interstellar medium parameters and Voyager probe measurements.

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TL;DR
How far will Voyager 1 deviate from straight-line motion over 100–1000 years due to interstellar gas/dust? Order-of-magnitude only. Has this been calculated?
I’m looking for order-of-magnitude bounds on how much Voyager 1’s trajectory would depart from a constant-velocity inertial extrapolation over long time scales (100, 500, 1000 years).

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Two separate quantities:
  1. Cross-track deviation
    Lateral displacement relative to a straight-line extrapolation.
  2. Along-track lag
    Distance difference due to cumulative slowing.
Assume (adjust if better values exist):
  • Mass ≈ 730 kg
  • Effective cross-section ≈ 10.75 m² (3.7 m antenna dish)
  • Speed ≈ 17 km/s
  • Neutral hydrogen density ≈ 0.1 cm⁻³
  • Dust-to-gas mass ratio ≈ 1%

I’m not looking for precise ephemerides - just whether the drift is on the order of meters, kilometers, 10³ km, etc., after ~10³ years.

Has this already been calculated in the literature, or is a back-of-envelope estimate the right approach here?
 

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Not that I can answer your question, but as I understand it, our knowledge of the interstellar medium is very much based on measurements made via Voyager 1 and 2. I am not aware if the range and range-rate profiles of the probes was/are factored into these models, but considering how minute effects can be and still are measured (e.g. the thermal Pioneer anomaly) I would expect a model of the Voyager probes non-gravitational interactions in the ISM to have been established to some level of detail as a part of this research. I would also expect that any cross-track drift, if measurable at all, to be many orders of magnitude more uncertain than the in-track range-rate.

Edit: fixed wording.
 
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With your assumptions, the acceleration due to gas (or gas+dust, a 1% effect isn't important here) is ##\frac{v^2\rho A}{m} = 7\cdot 10^{-16} \frac{m}{s^2}##. Over 100 years such an acceleration leads to a displacement of 3.5 km, over 1000 years it leads to a displacement of 350 km along its trajectory. Compare this to the 500 billion km it travels in that time. The path is not a straight line due to gravity, which effectively gives it a bit of displacement orthogonal to its motion as well, but that's a tiny higher order effect.
 
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