1. 0.16 N
The weight of a man on the surface of asteroid is equal to the gravitational force exerted on the man:
![F=G(Mm)/(r^2)](https://img.qammunity.org/2020/formulas/physics/middle-school/c5j8ee2f31m91gkcvriqi5k68op55s29ti.png)
where
G is the gravitational constant
is the mass of the asteroid
m = 100 kg is the mass of the man
r = 2.0 km = 2000 m is the distance of the man from the centre of the asteroid
Substituting, we find
![F=(6.67\cdot 10^(-11)m^3 kg^(-1) s^(-2))((8.7\cdot 10^(13) kg)(110 kg))/((2000 m)^2)=0.16 N](https://img.qammunity.org/2020/formulas/physics/high-school/9oq51io031uluhi6xp19at7uwl4sqf30zw.png)
2. 1.7 m/s
In order to stay in orbit just above the surface of the asteroid (so, at a distance r=2000 m from its centre), the gravitational force must be equal to the centripetal force
![m(v^2)/(r)=G(Mm)/(r^2)](https://img.qammunity.org/2020/formulas/physics/high-school/jsqgbe22wd19a6jgfaycu9e5rgu4xjytqm.png)
where v is the minimum speed required to stay in orbit.
Re-arranging the equation and solving for v, we find:
![v=\sqrt{(GM)/(r)}=\sqrt{((6.67\cdot 10^(-11) m^3 kg^(-1) s^(-2))(8.7\cdot 10^(13) kg))/(2000 m)}=1.7 m/s](https://img.qammunity.org/2020/formulas/physics/high-school/i9yuwf6fm5lnatmrfz0ktllibquwpt9fjr.png)