ICLO-5] 51 Peg is a star in our galaxy, similar to the Sun, In 1005, two ewiss astronomers discovered a planet around R. was the the Sun. The planet is caled 51 Peg b, on a crcular orbit the semimajor axis of the orbit is 0.05211 AU. The mass of the 51 Peg (the star) is 1.054 Mass of the Sun. Calculate the orbital period of the planet. Neglect the mass of the planet in your calculation. Given: G-6.67408 1011 m ko12 Mass of the Sun = 1,988,500 x 104 ko G (m, +m2) 1 AU - 1.5 x 108 km O -4.3 days O-378911 days 0:1,644.242 days. 0142 x 10 days.
ICLO-5] 51 Peg is a star in our galaxy, similar to the Sun, In 1005, two ewiss astronomers discovered a planet around R. was the the Sun. The planet is caled 51 Peg b, on a crcular orbit the semimajor axis of the orbit is 0.05211 AU. The mass of the 51 Peg (the star) is 1.054 Mass of the Sun. Calculate the orbital period of the planet. Neglect the mass of the planet in your calculation. Given: G-6.67408 1011 m ko12 Mass of the Sun = 1,988,500 x 104 ko G (m, +m2) 1 AU - 1.5 x 108 km O -4.3 days O-378911 days 0:1,644.242 days. 0142 x 10 days.
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![(CLO-5] 51 Peg is a star in our galaxy, similar to the Sun. In 1005, two ewiss astronomers discovered a planet around Rt was the
the Sun.
The planet is called 51 Peg b, on a dircular orbit the semi-major axis of the orbit is 0.05211 Au.
The mass of the 51 Peg (the star) is 1.054 Mass of the Sun.
Calculate the orbital period of the planet. Noglect the mass of the planet in your calculation.
Given:
G-6.67408 - 1011 m³ ko*12
Mass of the Sun = 1,988,500 x 1024 kg
G (m,+m)
1 AU » 1,5 x 108 km
O-4.3 days
O- 376911 days
0:1,644.242 days.
0142x 1011 days.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F0ff4fa38-41e9-49bd-973c-85c7e735a976%2F796e19ac-2221-4799-b636-5a30fa7a46f0%2Fsettkn_processed.jpeg&w=3840&q=75)
Transcribed Image Text:(CLO-5] 51 Peg is a star in our galaxy, similar to the Sun. In 1005, two ewiss astronomers discovered a planet around Rt was the
the Sun.
The planet is called 51 Peg b, on a dircular orbit the semi-major axis of the orbit is 0.05211 Au.
The mass of the 51 Peg (the star) is 1.054 Mass of the Sun.
Calculate the orbital period of the planet. Noglect the mass of the planet in your calculation.
Given:
G-6.67408 - 1011 m³ ko*12
Mass of the Sun = 1,988,500 x 1024 kg
G (m,+m)
1 AU » 1,5 x 108 km
O-4.3 days
O- 376911 days
0:1,644.242 days.
0142x 1011 days.
![[CLO-5] 51 Peg is a star in our galaxy, simllar to the Sun. In 1995, two swiss astronomers discovered a planet
The planet is called 51 Peg b.
The orbit of the planet is circular.
Which of the following statements is correct?
O a. 51 Peg b is faster when it is at the perihelion than when it is at the aphelion.
a.
O b.51 Peg b has a constant speed on its orbit.
Oc. 51 Peg b is slower when it is at the perihelion than when it is at the aphelion.
O d. We can not comment of the variation of the speed of a planet on its orbit if we do not know the ma!](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F0ff4fa38-41e9-49bd-973c-85c7e735a976%2F796e19ac-2221-4799-b636-5a30fa7a46f0%2Fuckkbal_processed.jpeg&w=3840&q=75)
Transcribed Image Text:[CLO-5] 51 Peg is a star in our galaxy, simllar to the Sun. In 1995, two swiss astronomers discovered a planet
The planet is called 51 Peg b.
The orbit of the planet is circular.
Which of the following statements is correct?
O a. 51 Peg b is faster when it is at the perihelion than when it is at the aphelion.
a.
O b.51 Peg b has a constant speed on its orbit.
Oc. 51 Peg b is slower when it is at the perihelion than when it is at the aphelion.
O d. We can not comment of the variation of the speed of a planet on its orbit if we do not know the ma!
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