Macmillan Learning A day on a distant planet observed orbiting a nearby star is 72.5 hr. Also, a year on the planet lasts 89.7 Earth days. In other words, for the purposes of unit conversion, there are 24 hr in a day, 60 min in an hour, and 60 s in a minute, as it would for astronomers on Earth observing the planet. Calculate the average angular speed of the planet about its own axis of rotation in radians per second with the second as measured on Earth. speed of rotation: rad/s Calculate the average angular speed of the planet as it travels around its neighboring star, with the second as measured on Earth.

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ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
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**Calculating Angular Speeds on a Distant Planet**

A day on a distant planet observed orbiting a nearby star is 72.5 hours. Additionally, a year on the planet lasts 89.7 Earth days. For unit conversion purposes, a day is considered 24 hours, an hour is 60 minutes, and a minute comprises 60 seconds, as it would for astronomers on Earth observing the planet.

**Objective 1: Calculate the Average Angular Speed of the Planet About Its Own Axis of Rotation**

- **Speed of Rotation:** \( \_\_\_\_\_\_\_\_ \) rad/s

**Objective 2: Calculate the Average Angular Speed of the Planet as It Travels Around Its Neighboring Star**

- **Speed of Orbit:** \( \_\_\_\_\_\_\_\_ \) rad/s

These calculations are crucial for understanding the rotational dynamics and orbital mechanics of celestial bodies.
Transcribed Image Text:**Calculating Angular Speeds on a Distant Planet** A day on a distant planet observed orbiting a nearby star is 72.5 hours. Additionally, a year on the planet lasts 89.7 Earth days. For unit conversion purposes, a day is considered 24 hours, an hour is 60 minutes, and a minute comprises 60 seconds, as it would for astronomers on Earth observing the planet. **Objective 1: Calculate the Average Angular Speed of the Planet About Its Own Axis of Rotation** - **Speed of Rotation:** \( \_\_\_\_\_\_\_\_ \) rad/s **Objective 2: Calculate the Average Angular Speed of the Planet as It Travels Around Its Neighboring Star** - **Speed of Orbit:** \( \_\_\_\_\_\_\_\_ \) rad/s These calculations are crucial for understanding the rotational dynamics and orbital mechanics of celestial bodies.
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