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Journal of Physics Special Topics An undergraduate physics journal

P2 2 Voyager 1: 43 Young

J. Duggan, G. Gillan, L. Meehan, A. Tyrrell Department of Physics and , University of Leicester, Leicester, LE1 7RH November 26, 2020

Abstract can measurably dilate for objects which are in gravitational fields or are moving at high . Here we investigate the effects relativity has on the and passing of time on the Voyager 1 spacecraft. The experienced due to the of the spacecraft was calculated as 50 ms/yr and compared with the time dilation due to gravity at ’s surface of 22 ms/yr. The net dilation for Voyager 1 was therefore calculated as 1.23 s.

Introduction ∆t0 = γ∆t (1) Relativistic effects are rarely considered in daily life as most of us do not travel anywhere where, near the . However, in there 1 is a lot of room for acceleration without air re- γ = (2) q v2 sistance or other limiting factors experienced on 1 − c2 Earth. Spacecraft travel at high speeds in order to cross the vast distances of space in as little Equation (1) tells us how long it takes for a pe- time as possible but currently still take many riod of time to pass for observers in another ref- years to reach their destinations. As we make erence frame. In this scenario, the equation is used to calculate how much time has passed for faster and faster spacecraft, relativistic effects 0 will increase and potentially become significant. the Voyager craft, ∆t , compared with the time In this paper, we investigate the effects of time that has passed for a stationary observer, ∆t. dilation on the Voyager 1 spacecraft, currently The speed of light is represented by c and veloc- travelling at ∼ 17 km/s [1] out of our solar sys- ity is represented by v. tem, and compare it to the passage of time at The equation used is derived from Earth, which is also dilated by its gravitational , specifically the Schwarzschild field. metric, which describes space-time in the vicin- ity of a non-rotating massive sphere. This equa- Theory tion is used to calculate the time dilation for observers inside the gravitational influence of a Time dilation occurs between an observer in planet, in this case Earth. an inertial frame and an object/person moving r relative to them. It can be calculated from the 2GM t = t 1 − (3) Lorentz transformations [2]. 0 f rc2 Here, M is the of earth, r is the separa- however be slightly inaccurate as it is the time tion from the centre of the earth, and c and G passing at a theoretically infinite distance from have their usual meanings. For simplicity, the Earth where its gravitational field has no effect. Earth is assumed to be non-rotating which allows For the purposes of this paper we take the dif- equation (3) to be used. Here, t0, represents the ference to be negligible. between events for an observer close The combined γ0 factor works out to be to the massive sphere (Earth in this case), and 0.9999999991 for Earth and Voyager meaning for tf represents the between events every second Earth experiences, Voyager experi- for an observer at an infinite distance where a ences 0.9999999991 . This period of time would tick one second per second of coor- is larger than when compared with the station- dinate time. ary observer as the effect of Earth’s gravity slows To calculate the time dilation of the Voyager down time also. 1 spacecraft and compare it to that in Earth’s Conclusion gravity, equations (1) and (3) can be combined Since its launch, Voyager 1 has aged 2.2 sec- [3] to create a new gamma factor γ0 shown in onds less than a stationary observer on Earth. In equation (4): this same time, the Earth has aged 0.95 seconds

q v2 less than a point in the universe under no influ- 1 − 2 γ0 = c (4) ence of gravity. However when compared to each q 2GM other, Voyager experiences time the slowest, only 1 − 2 rc experiencing 1.23 s fewer over 43 years of Earth This γ0 combines the time dilation effects of grav- time. This shows that effects due to Earth’s ity and velocity across reference frames so that gravity and the speeds our spacecraft travel do both influences can be accounted for when cal- not have significant relativistic consequences and culating time dilation for Voyager 1. therefore shouldn’t cause any problems. In or- Results and Discussion der to make time dilation a significant factor, we Using equations (1) and (2), we calculated would need to launch spacecraft at much higher that a stationary observer would see Voyager 1’s speeds or live within a gravitational field similar time passing at a rate of 0.9999999984 seconds to that produced by a . per second locally. This means that, as Voyager 1 References is not moving at a significant fraction of c, the di- [1] https://voyager.jpl.nasa.gov/mission/ lation is almost insignificantly small, losing only status/ [Accessed 27 October 2020] 2.2 s over 43 years at a rate of ∼ 0.05 s/yr. The effects of time dilation due to Earth’s [2] Tipler P. A., Mosca, G., 2008. Time Dila- gravity were calculated with equation (3) (us- tion. In: Physics for Scientists and Engineers: ing Earth’s radius and mass [4]) and we found Sixth Edition. New York: W. H. Freeman that for every second passing on Earth, we would and Company, p. R-5. only measure 0.9999999993 seconds passing out [3] A.Conte, Combination of time dilation and in deep space where the gravity is insignificant. gravitational time dilation (2020) If Voyager 1 was far away from Earth and sta- tionary relative to Earth, over the 43 years since [4] https://en.wikipedia.org/wiki/Earth launch we would measure it as ∼ 0.95 seconds [Accessed 27 October 2020] younger than at Earth. This is a smaller dif- ference in time period when compared with the dilation caused by Earth due to the relatively small mass of our planet. This number would