FzzXIP25S'_[Ŕ>)T?€3˙“˙˙HomeBpC|Ă˙˙MainBpCLĂ ZoomD\jŞC0Ă ›ŕ?LĚÁ'$x HHđ@˙ě˙îRd(ühh° @d'˙œ˙Ś š’˙˙MainBpCLĂ ˙˙RÜV;Ł× < ¨€(?€;Ł× ?€< ¨?€?€˙˙U˙˙'šÜ”…ƒŒb A‹˙˙ˆSystem Center of Mass˙˙'—Ÿ–ĽMkg?€?€Ÿ–ĽDm?€?€Ÿ–ĽĄrad?€?€Ÿ–ĽCA?€?€Ÿ–ĽKK?€?€Ÿ–Ľmmole?€?€Ÿ–ĽLcd?€?€Ÿ–ĽTs?€?€Ÿ–ÄÄŕN?€?€Ÿ–ENŕJ?€?€Ÿ–WWĐW?€?€Ÿ–CHC?€?€Ÿ–˝˝ŕŕ˝?€?€Ÿ–VlĐđV?€?€Ÿ–RVń?€?€Ÿ–Hzđ?€?€Ÿ–Spđ?€?€˜đ/s?€?€ńrad/s?€?€ŕm/s^2?€?€đm/s?€?€m^2?€?€kg m^2?€?€óŕ N m^2/kg^2?€?€óŕ N m^2/kg^2?€?€óŕ N m^2/kg^2?€?€óŕ N m^2/kg^2?€?€óŕ N m^2/kg^2?€?€óŕ N m^2/kg^2?€?€óŕ N m^2/kg^2?€?€óŕ N m^2/kg^2?€?€˙˙'Ž@ frame()=960˙˙' ˙˙'í˙˙'AőĂ?€q˙˙?€'9-self.mass*( 1.0000000e+0)/sqr(self.p-other.p)*other.massŒb A‹˙˙ˆ˙˙'î˙˙' Pö!q˙˙?€'Œb A‹˙˙ˆ˙˙'ě˙˙'@ @ q angle(self.v)?€'Œb A‹˙˙ˆ˙˙'ď˙˙'!q˙˙?€'Œb A‹˙˙ˆ˙˙'‚ÔˇˇÝk¢>LĚÍ>¸>¸˙˙˛?˙˙˙?˙˙˙^˙˙dŠŒ°¸ş— ;đם‘Ŕř5*mass[6].mass/mass[1].massBČBG˙ý˙„ƒŒbA‹ˆSun•˙˙]‰‚ľ`Years@ff Apparent Weight/Newtonian Weight>ˇZüťŁ× ?LĚÍÔŕ‰ä bA‹ˆ#Apparent Weight of Small Red Square@time/2.2$1361*|normalforce(6,2)|/mass[6].mass•˙˙˛>LĚĚ>LĚĚ^Ô°Ŕ?mżžL–?LĚÁ>ä[‚ŔŸčAŸ˙ó Input[11];Znr?>™™šĎÔ„ƒŒb A‹ˆ Planet X• ˙˙Ľ=_—9‡@;–R<(ôźĐ.€=MŰź§8€˝Mî˙˙ąÝk¢°Ŕ:/ѽ@:hÍżšKŽŔVw6AŸű~7'ĹŹ-zz=ĚĚÍCŒÝk¢b A‹˙˙ˆPolygon˙˙y? ˙˙˙˙˙˙‰Yqb‹ˆButton 5˙˙y?˙˙˙˙˙˙‰YŠb‹ˆButton 7˙˙yxî˙˙˙˙˙˙‰mqb‹ ˆButton 8˙˙ Y}˙ţZÖThe graph shows the ratio of the apparent weight of the tiny red object "standing" on Planet X to its Newtonian gravitational interaction force with Planet X. This is identical to the ratio of the reading of the red object's accelerometer to the Newtonian gravitational field strength at its position. When and why does the ratio have maxima and minima? When and why are the minima smallest? When and why are the maxima largest? Why is the ratio always less than 1?‰$b A‹ ˆText˙˙ x˙˙?€'gg˙˙˙˙S€ ‚ Œ Œ ˙˙˙˙S€ A S€H AHv ˙˙˙˙˙˙˙˙H Ą– Ąš 3=, Geneva .+'Š 1997  —Ą– Ąš+ )?i* A. J. Mallinckrodt  —Ą– Ąš˙ű$ 5A[* Cal Poly Pomona —Ą– Ąš˙ű-  h ( Tidal Effects —  ƒ˙{T‰nb A‹ ˆPicture˙˙ \?€?™š@g<P‰˜\b A‹ ˆRelative mass of Planet X@ Input[11]˙˙ yXőý˙˙˙˙˙˙‰ąb‹ ˆ Main View˙˙ y‰őü˙˙˙˙˙˙‰Çfb‹˙˙ˆFrame of Planet X˙˙