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Hot Jupiters. In 2004 astronomers reported the discovery of a large Jupiter-sized planet orbiting very close to the star HD179949 (hence the term 鈥渉ot Jupiter鈥). The orbit was just19 the distance of Mercury from our sun, and it takes the planet only3.09days to make one orbit (assumed to be circular). (a) What is the mass of the star? Express your answer in kilograms and as a multiple of our sun鈥檚 mass. (b) How fast (in km>s) is this planet moving?

Short Answer

Expert verified

a)The mass of the star is 2.211030鈥塳驳, andmstar=1.11msun

b) The planet is moving at a speed of 1.51105鈥尘/s.

Step by step solution

01

Identification of the given data

  • The orbit is19 the distance of the Mercury from the sun.
  • The planet takes about3.09 making one orbit.
02

 Step 2: Significance of the Kepler’s third law in identifying the mass of the star and speed of the planet

This law illustrates that a planet鈥檚 orbital period鈥檚 square is equal to its orbit鈥檚 鈥渟emi-major axes鈥.

The product of the cube of the radius and the Kepler's constant, along with the time period, will provide the star's mass. Moreover, dividing the perimeter of the star by the time period gives the star's speed.

03

Determination of the mass and also the speed of the star

a) From Kepler鈥檚 third law, the orbital period of the star can be expressed as:

T=2蟺谤3/2Gmstarmstar=42r3T2G

Here, T is the planet's orbital period, which is3.09鈥塪补测蝉=2.67105鈥塻r is the orbit radius of theearth 5.791010鈥尘9=6.43109m. The value of G, which is the gravitational constant is 6.671011N.m2kg2.

Substituting the values in the above equation, we get,

mstar=4蟺2(6.43脳109鈥尘)3(2.67脳105鈥塻)26.67脳10-11N.m2kg2mstar=2.211030鈥塳驳

Hence, the mass of the star is 2.211030鈥塳驳.

Apart from that, it has been observed that mstarmsun=1.11, hence,mstar=1.11msun

b) The orbital velocity of the planet is expressed as:

v=2蟺谤T

Here v is the orbital velocity, r is the orbital radius of the planet,6.43109鈥尘 and T is the earth's orbital period 2.67105鈥塻.

Substituting the values in the above equation, we get-

v=2(6.43109鈥尘)2.67105鈥塻v=1.51105鈥塻

Thus, the planet is moving at a speed of 1.51105鈥塻.

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