You've got radius You know solar mass I assume you know the value of newton's constant In circular motion the gravitational force of sun is the centripetal of earth Your circular equation is a bit dodged though
You've got radius You know solar mass I assume you know the value of newton's constant In circular motion the gravitational force of sun is the centripetal of earth Your circular equation is a bit dodged though
the i subbed in values 6.67x10^-11 x 5.97x10^24 divided by the radius in m 1.5x10^11 and rooted and i got 51.52 but the answer should have been 3.0 × 10^4ms–1
the i subbed in values 6.67x10^-11 x 5.97x10^24 divided by the radius in m 1.5x10^11 and rooted and i got 51.52 but the answer should have been 3.0 × 10^4ms–1
I got ~29.5 kms^-1; something you should memorise actually it shows up fairly frequently iirc. Anyway, your M is wrong. What's that 5.97? The mass of the sun is 1.989x10^30 kg.
I got ~29.5 kms^-1; something you should memorise actually it shows up fairly frequently iirc. Anyway, your M is wrong. What's that 5.97? The mass of the sun is 1.989x10^30 kg.
ah i was using the earth's mass, how do you know when to use the sun's mass or earth's, i assumed it was the earth since the question said earth's speed
ah i was using the earth's mass, how do you know when to use the sun's mass or earth's, i assumed it was the earth since the question said earth's speed
You just need to know the equations and the physics behind them. If you know that, you'll know which numbers to push through them.
I.e. in this case you did the force on the earth from the sun r2GM⊙×m⊕
is equivalent to the centripetal force on the earth necessary for circular motion rm⊕v2
cancelled out the
Unparseable latex formula:
m_\quad
and put in your values for G,M⊙,r which are ~6.67e-11,1.989e30,1.5e11/astronomical-unit.
You just need to know the equations and the physics behind them. If you know that, you'll know which numbers to push through them.
I.e. in this case you did the force on the earth from the sun r2GM⊙×m⊕
is equivalent to the centripetal force on the earth necessary for circular motion rm⊕v2
cancelled out the
Unparseable latex formula:
m_\quad
and put in your values for G,M⊙,r which are ~6.67e-11,1.989e30,1.5e11/astronomical-unit.
Could you also please help me with this q? the answer is A how do you go about these type of question
Two satellites, P and Q, of the same mass, are in circular orbits around the Earth. The radius of the orbit of Q is three times that of P. Which one of the following statements is correct? A The kinetic energy of P is greater than that of Q. B The weight of P is three times that of Q. C The time period of P is greater than that of Q. D The speed of P is three times that of Q.
Could you also please help me with this q? the answer is A how do you go about these type of question
Two satellites, P and Q, of the same mass, are in circular orbits around the Earth. The radius of the orbit of Q is three times that of P. Which one of the following statements is correct? A The kinetic energy of P is greater than that of Q. B The weight of P is three times that of Q. C The time period of P is greater than that of Q. D The speed of P is three times that of Q.
If it's a new Q I recommend making a new post (makes it easier for future people looking for the same answer)