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The total intensity of light measured on earth, from an ecliptic binary, is plotted in the figure as a function of time (it's called a light curve). Careful measurements indicate that the intensities of the incident light from the stars corresponding to the minima are respectively 90 and 63 percent of the maximum intensity, received both Io, temperatures of two stars in an eclipsing binary are T1 and T2 (T1 > T2), and the corresponding radii (R1 > R2), respectively. from stars.Surface R1 and R2 аге Find the ratio T1/T2. Round you answer to two significant figures. 1.0 0.8 1|1, =0.90 0.6 04 11, =0.63 0.2 1.0 2.0 3.0 4.0 5.0 6.0 Time (days)

The total intensity of light measured on earth, from an ecliptic binary, is plotted in the figure as a function of time (it's called a light curve). Careful measurements indicate that the intensities of the incident light from the stars corresponding to the minima are respectively 90 and 63 percent of the maximum intensity, received both Io, temperatures of two stars in an eclipsing binary are T1 and T2 (T1 > T2), and the corresponding radii (R1 > R2), respectively. from stars.Surface R1 and R2 аге Find the ratio T1/T2. Round you answer to two significant figures. 1.0 0.8 1|1, =0.90 0.6 04 11, =0.63 0.2 1.0 2.0 3.0 4.0 5.0 6.0 Time (days)

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The total intensity of light measured on earth, from an ecliptic binary, is plotted in the figure as a function of time (it's called a light curve). Careful measurements indicate that the intensities of the incident light from the stars corresponding to the minima are respectively 90 and 63 percent of the maximum intensity, received both Io, temperatures of two stars in an eclipsing binary are T1 and T2 (T1 > T2), and the corresponding radii (R1 > R2), respectively. from stars.Surface R1 and R2 аге Find the ratio T1/T2. Round you answer to two significant figures. 1.0 0.8 1|1, =0.90 0.6 04 11, =0.63 0.2 1.0 2.0 3.0 4.0 5.0 6.0 Time (days)
Transcribed Image Text:The total intensity of light measured on earth, from an ecliptic binary, is plotted in the figure as a function of time (it's called a light curve). Careful measurements indicate that the intensities of the incident light from the stars corresponding to the minima are respectively 90 and 63 percent of the maximum intensity, received both Io, temperatures of two stars in an eclipsing binary are T1 and T2 (T1 > T2), and the corresponding radii (R1 > R2), respectively. from stars.Surface R1 and R2 аге Find the ratio T1/T2. Round you answer to two significant figures. 1.0 0.8 1|1, =0.90 0.6 04 11, =0.63 0.2 1.0 2.0 3.0 4.0 5.0 6.0 Time (days)
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