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With a calculator, we have a handy way to estimate $ \mu $, if we remember there are (100 + 3) leap years per 400 years ; 1 year = 365.2575 days = 31558248 seconds, 1 AU = 149.6e9 meters, estimated $\mu$ = 1.327176698e20 m^3^/s^2^. The book value is 1.32712440018e20 m^3^/s^2^ (estimate is 39 ppm high), a year is 365.256363004 days (estimate is 3 ppm high), and earth's semimajor axis is 1.49598023e9 meters (estimate is 13 ppm high). Which leaves a 6 ppm discrepancy, but pretty good for semi-POMA numbers. With a calculator, we have a handy way to estimate $ \mu $ to 4 decimal places.

R
emember that there are (100 + 3) leap years per 400 years ; 1 year = 365.2575 days = 31558248 seconds, 1 AU = 149.6e9 meters, estimated $\mu$ = 1.327176698e20 m^3^/s^2^. The book value is 1.32712440018e20 m^3^/s^2^ (estimate is 39 ppm high), a year is 365.256363004 days (estimate is 3 ppm high), and earth's semimajor axis is 1.49598023e9 meters (estimate is 13 ppm high). Which leaves a 6 ppm discrepancy, but pretty good for semi-POMA numbers.

Stadyshell Falling

Without light pressure or horizontal velocity, how long would it take for a stadyshell to fall into the sun?

Falling into the sun is an orbit with an aphelion of the starting height r = 50 AU, and a perhelion of 0. The semimajor axis a = r2 , and the eccentricity is 1.0. The falling time is half the orbital period for this orbit, T=r38 .

We could look up - but we can calculate it pretty accurately - without a calculator! The earth is in an orbit with a semimajor axis of 1 AU, and the period is a year. so (1year)=2(1AU)3 . Solving, =42AU3year2 . So the falling time is:

T=125000AU3(322AU3year2)=12500032=(1252)2  years. So T = 62.5 years. Which would be exact if the earth had a 1 AU semimajor axis, which it does not, see below.

With a calculator, we have a handy way to estimate \mu to 4 decimal places.

Remember that there are (100 + 3) leap years per 400 years ; 1 year = 365.2575 days = 31558248 seconds, 1 AU = 149.6e9 meters, estimated \mu = 1.327176698e20 m3/s2. The book value is 1.32712440018e20 m3/s2 (estimate is 39 ppm high), a year is 365.256363004 days (estimate is 3 ppm high), and earth's semimajor axis is 1.49598023e9 meters (estimate is 13 ppm high). Which leaves a 6 ppm discrepancy, but pretty good for semi-POMA numbers.

How long does it take to fall half way down?

We can project the zero-width elliptical orbit on a unit circle, and compute the area swept halfway through the circle and ratio that to a half circle. The pie shaped area swept is half the total area, and the triangle to that halfway point is ( 1/2 ) / ( \pi / 2 ) = (1/\pi ) , so the time is 62.5 years * 1/2 + 1/pi = 51.14 years . Other times can be solved similarly, with trigonometry. We can approximate with constant gravity for the first few years of drop. At 50 AU, g = $ ( \pi2 / 625 ) {AU}/{year}2, so 1 year of falling is 0.008 AU, and 5 years of falling is 0.2 AU. Not much, and a 0.2% increase in temperature at black body equilibrium (except we are sideways for this to happen, and the thinsat is not getting any sunlight, and closer to 2.7 K ).

StadyshellFalling (last edited 2015-11-16 23:04:32 by KeithLofstrom)