| 10 | | || '''ke(r)''' || '''Distance (pc)''' || '''Error (%)'''|| |
| 11 | | || 10*freefall || 6.8x10^-7^ || 30 || |
| 12 | | || 100*freefall || 7.4x10^-6^ || 30 || |
| 13 | | || 1000*freefall || 7.5x10^-5^ || 30 || |
| 14 | | || 10*freefall || .00002 || .01 || |
| 15 | | || 100*freefall || .0002 || .01 || |
| 16 | | || 1000*freefall || .002 || .01 || |
| | 12 | |
| | 13 | || '''ke(r)''' || '''Error (%)''' || '''Distance (pc)'''|| |
| | 14 | || 10*freefall || 30 || 6.8x10^-7^ || |
| | 15 | || 10*freefall || .01 || .00002 || |
| | 16 | || 100*freefall || 30 || 7.4x10^-6^ || |
| | 17 | || 100*freefall || .01 || .0002 || |
| | 18 | || 1000*freefall || 30 || 7.5x10^-5^ || |
| | 19 | || 1000*freefall || .01 || .002 || |
| | 20 | |
| | 21 | |
| | 22 | Now, what if a gas parcel started from rest, a distance r away from the star surface? Now we are solving, |
| | 23 | |
| | 24 | [[latex($-\frac{G*M}{r}+\frac{G*M}{R} = .99 (\frac{GM}{R})$)]] |
| | 25 | |
| | 26 | [[latex($-\frac{G*M}{r}+\frac{G*M}{R} = .70 (\frac{GM}{R})$)]] |
| | 27 | |
| | 28 | || '''ke(r)''' || '''Error (%)''' || '''Distance (pc)'''|| |
| | 29 | || 0 || .01 || 2.2x10^-6^ || |
| | 30 | || 0 || 30 || 7.5x10^-8^ || |
| | 31 | |
| | 32 | |
| | 33 | Lastly, what if the parcel was moving, however, it was moving ''slower'' than freefall? Now ke(r) will be a fraction of the freefall energy in the table below. In particular, what if ke(r) was 1/2, 1/5, 1/10 the freefall kinetic energy... at what distance, r, would I see a 0.01% error? What about a 30% error? |
| | 34 | |
| | 35 | [[latex($ke(r)-\frac{G*M}{r}+\frac{G*M}{R} = .99 (\frac{GM}{R})$)]] |
| | 36 | |
| | 37 | [[latex($ke(r)-\frac{G*M}{r}+\frac{G*M}{R} = .70 (\frac{GM}{R})$)]] |
| | 38 | |