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I was doing some back-of-a-postage-stamp calculations on high-isp interstellar spacecraft earlier and realised something. If I design a spaceship which according to the rocket equation has a very high Delta-V, close or even beyond the speed of light (in my calculations it was 6.7 million km/s or 22c), how do you calculate what speed that spacecraft can actually accelerate to? Obviously a spacecraft with a Delta-v of 6.7 million km/s cannot actually accelerate to that speed (with it being faster-than-light and all), but how fast could it get?

For those wondering, here’s my math on the example craft I referenced:

Assuming photon drive powered by 100% efficient antimatter reactions, 1 exawatt of power to the drive = 3 million kilonewtons of thrust or 337,000 tons thrust. This requires 1.7 million tons of antimatter (& 1.7 million tons of matter, 3.4 million total), and can fire for 10 years.

Assuming mass fraction of 90%

TWR of ~0.08

Delta V of ~6.7 million km/s (22c)

Organic Marble
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1 Answers1

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In the case where the spacecraft can achieve relativistic speeds and no gravity is involved, $\Delta v$ is actually $c$ times the maximal change of rapidity which can be achieved. So the maximal speed the spacecraft can accelerate to, starting from zero, is $c \tanh \frac{\Delta v}{c}$. For example, if the maximal rapidity is $22$, then the maximal speed is $c \tanh 22\approx 0.9999999999999999998c$.

Litho
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  • This is interesting! Is $\Delta v$ here just the traditional $v_e \log(m_i/m_f)$? Would this help me with my confusing here and is $\gamma$ needed or not? – uhoh Apr 03 '20 at 10:33
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    @uhoh Here, in general, $\Delta v$ is $T_s \ln(m_i/m_f)$, where $T_s$ is the total thrust per unit mass spent. In the case $v_e << c$, $T_s = v_e$, so $\Delta v = v_e \ln(m_i/m_f)$. In the case of relativistic $v_e<c$, I think that $\Delta v$ is still $v_e \ln(m_i/m_f)$, see my comments to the answer you linked to. – Litho Apr 03 '20 at 12:21
  • Thanks for looking into these! – uhoh Apr 03 '20 at 12:31