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词汇 periapsis
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Examples of periapsis


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As a planet approaches periapsis, the planet will increase in speed, or velocity.
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Particularly at each periapsis, the object experiences atmospheric drag, losing energy.
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For near-circular orbits, it is hard to find the periapsis in the first place (and truly circular orbits have no periapsis at all).
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The last time they were at periapsis was in 1836.
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The ecliptic longitudes of the periapsis of the satellite and the planet are locked.
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The initial, high eccentricity orbits may also be a source of gravitational waves, emitting a short burst as the compact object passes through periapsis.
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It had a periapsis of 171 km and an apoapsis of 3,524 km and an orbital period of 619 minutes.
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These variations are connected with the variations of the ring width, which is 19.7 km at the periapsis and 96.4 km at the apoapsis.
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When gradually making an elliptic orbit smaller, it means applying thrust each time when near the periapsis.
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With increasing release height the orbit becomes less eccentric as both periapsis and apoapsis increase, becoming circular at geostationary level.
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The angular rate is faster nearer periapsis and slower near apoapsis.
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Thereafter, the periapsis was allowed to rise to a maximum of and then fall, to conserve fuel.
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The point on the orbit closest to the attracting body is the periapsis.
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When gradually making an elliptic orbit larger, it means applying thrust each time when near the periapsis.
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So to get the most kinetic energy from the burn, the burn must occur at the vehicle's maximum velocity, at periapsis.
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Adding the argument of periapsis to the longitude of the ascending node gives the longitude of the periapsis.
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A line drawn from periapsis to apoapsis is the line-of-apsides.
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For the most efficient example mentioned above, targeting an inclination at apoapsis also changes the argument of periapsis.
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A straight line connecting the periapsis and apoapsis is the "line of apsides".
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