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Astronomers discover a planet orbiting a faraway star using the transit method, whereby the periodic dip in the intensity of the received starlight reveals the orbital period of the planet (the intensity drops when the planet blocks some of the starlight). By examining other characteristics of the star's light, the mass of the star is determined to be M = 6.5 × 10³¹ kg. 1.002 1.000 0.998 0.996 Estimate the planet's orbital period from the graph and use this number to calculate the planet's distance from the star (assume a circular orbit). 0.994 0.992 3 4 5 Time (days) G = 6.67 × 10-¹1 Nm²/kg² O Relative Brightness 0 2 r T exopla

Astronomers discover a planet orbiting a faraway star using the transit method, whereby the periodic dip in the intensity of the received starlight reveals the orbital period of the planet (the intensity drops when the planet blocks some of the starlight). By examining other characteristics of the star's light, the mass of the star is determined to be M = 6.5 × 10³¹ kg. 1.002 1.000 0.998 0.996 Estimate the planet's orbital period from the graph and use this number to calculate the planet's distance from the star (assume a circular orbit). 0.994 0.992 3 4 5 Time (days) G = 6.67 × 10-¹1 Nm²/kg² O Relative Brightness 0 2 r T exopla

Applications and Investigations in Earth Science (9th Edition)
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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6 Astronomers discover a planet orbiting a faraway star using the transit method, whereby the periodic dip in the intensity of the received starlight reveals the orbital period of the planet (the intensity drops when the planet blocks some of the starlight). By examining other characteristics of the star's light, the mass of the star is determined to be M = 6.5 × 10³¹ kg. 1.002 1.000 0.998 0.996 Estimate the planet's orbital period from the graph and use this number to calculate the planet's distance from the star (assume a circular orbit). 0.994 0.992 3 4 5 6 7 Time (days) G = 6.67 × 10-¹¹ N m²/kg² exoplanet Relative Brightness 0 1 2 r T Ө
Transcribed Image Text:6 Astronomers discover a planet orbiting a faraway star using the transit method, whereby the periodic dip in the intensity of the received starlight reveals the orbital period of the planet (the intensity drops when the planet blocks some of the starlight). By examining other characteristics of the star's light, the mass of the star is determined to be M = 6.5 × 10³¹ kg. 1.002 1.000 0.998 0.996 Estimate the planet's orbital period from the graph and use this number to calculate the planet's distance from the star (assume a circular orbit). 0.994 0.992 3 4 5 6 7 Time (days) G = 6.67 × 10-¹¹ N m²/kg² exoplanet Relative Brightness 0 1 2 r T Ө
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