A body revolved around the sun $27$ times faster then the earth what is the ratio of their radii
$ \frac{1}{3}$
$ \frac{1}{9}$
$ \frac{1}{27}$
$ \frac{1}{4}$
Let the speed of the planet at the perihelion Pin Figure be $v_{p}$ and the Sun-planet distance $SP$ be $r_{ P }$ Relate $\left\{r_{P}, v_{P}\right\}$ to the corresponding quantities at the aphelion $\left\{r_{A}, v_{A}\right\} .$ Will the planet take equal times to traverse $B A C$ and $C P B ?$
What does not change in the field of central force
Earth's orbit is an ellipse with eccentricity $0.0167$. Thus the earth's distance from the sun and speed as it moves around the sun varies from day-to-day. This means that the length of the solar day is not constant through the year. Assume that the earth's spin axis is normal to its orbital plane and find out the length of the shortest and the longest day. A day should be taken from noon to noon. Does this explain variation of length of the day during the year ?
Describe the method for drawing an ellipse and explain foci of ellipse, midpoint, semi major axis.
The distance between Sun and Earth is $R.$ The duration of year if the distance between Sun and Earth becomes $3R$ will be