Answer:
27h
Step-by-step explanation:
We can answer this problem with Kepler's third law:
![(T^2)/(a^3) =constant](https://img.qammunity.org/2020/formulas/physics/high-school/p30bkdquy26o6xcoa1oxvvq4k4s8a5tdu5.png)
where
is the period and
is the semi-major axis of an ellipse, but because the satellite's orbit is around the earth it must be a circular orbit, so that
becomes the radius
of a circle.
![(T^2)/(r^3) =constant](https://img.qammunity.org/2020/formulas/physics/high-school/76l0941pt2v1ybhmza60thy9wwltn3j7hn.png)
what this tells us is that the relationship between the first period with radius
must be equal to the second period when the radius is now 9 times the original (the second radius is
because the orbit is nine times larger):
We will have the following:
![(T_(1)^2)/(r^3) =(T_(2)^2)/((9r)^3)](https://img.qammunity.org/2020/formulas/physics/high-school/xxzd3ktn43vs2e552yt3srw82vhdhw2uqs.png)
is the original period: 1 hour
is the period of the second satellite.
and
![(9r)^3=729r^3](https://img.qammunity.org/2020/formulas/physics/high-school/zbv6f5w5tzxdrvpb8hq56wobb167ovodwj.png)
thus:
![((1h)^2)/(r^3) =(T_(2)^2)/(729r^3)](https://img.qammunity.org/2020/formulas/physics/high-school/jf54bqkxdeb0gakrsnolaixdxj9mb0pw1p.png)
Clearing for
![((1h)^2)/(r^3)(729r^3) ={T_(2)^2}](https://img.qammunity.org/2020/formulas/physics/high-school/jnmsmt04n5nlplfbux6g4o0gs4gd4pzsrq.png)
![729=T_(2)^2](https://img.qammunity.org/2020/formulas/physics/high-school/duwe8xtil0rsdkm7ky7mbabcipmqhhw1zz.png)
![√(729)=T_(2)](https://img.qammunity.org/2020/formulas/physics/high-school/eh54majk1cxv0frujh64ygmnscny19am7g.png)
![27=T_(2)](https://img.qammunity.org/2020/formulas/physics/high-school/ollfy5k8ob3k8wslgz77oxz9sa7zwbw987.png)
The period of the second satellite is 27 hours