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What is the angular diameter of Saturn (in degrees) as seen from the surface of Rhea?

What is the angular diameter of Saturn (in degrees) as seen from the surface of Rhea?

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What is the angular diameter of Saturn (in degrees) as seen from the surface of Rhea?

**Celestial Profile: SATURN** --- **MOTION** - **Average distance from the Sun**: 9.58 AU (1.43 × 10⁹ km) - **Eccentricity of orbit**: 0.056 - **Inclination of orbit to ecliptic**: 2.5° - **Orbital period**: 29.5 years - **Rotation period (sidereal)**: 10.57 hours - **Inclination of equator to orbit**: 26.7° --- **CHARACTERISTICS** - **Equatorial diameter**: 1.21 × 10⁵ km (945 Earth diameters) - **Mass**: 5.68 × 10²⁶ kg (95.2 Earth masses) - **Average density**: 0.69 g/cm³ - **Gravity at cloud tops**: 1.1 Earth gravities - **Escape velocity**: 35.5 km/s (3.2 × Earth's escape velocity) - **Temperature at cloud tops**: 95 K (−290°F) - **Albedo**: 0.34 - **Oblateness**: 0.098
Transcribed Image Text:**Celestial Profile: SATURN** --- **MOTION** - **Average distance from the Sun**: 9.58 AU (1.43 × 10⁹ km) - **Eccentricity of orbit**: 0.056 - **Inclination of orbit to ecliptic**: 2.5° - **Orbital period**: 29.5 years - **Rotation period (sidereal)**: 10.57 hours - **Inclination of equator to orbit**: 26.7° --- **CHARACTERISTICS** - **Equatorial diameter**: 1.21 × 10⁵ km (945 Earth diameters) - **Mass**: 5.68 × 10²⁶ kg (95.2 Earth masses) - **Average density**: 0.69 g/cm³ - **Gravity at cloud tops**: 1.1 Earth gravities - **Escape velocity**: 35.5 km/s (3.2 × Earth's escape velocity) - **Temperature at cloud tops**: 95 K (−290°F) - **Albedo**: 0.34 - **Oblateness**: 0.098
**Table A-11: Principal Satellites of the Solar System** This table provides detailed information on the principal satellites of various planets in the Solar System. It includes data about each satellite's radius, distance from its primary planet, orbital period, orbital eccentricity, and orbital inclination. **Columns**: 1. **Primary**: The planet around which the satellite orbits. 2. **Satellite**: The name of the satellite. 3. **Radius (km)**: The radius of the satellite in kilometers. 4. **Distance from Primary (10^3 km)**: The average distance from the satellite to its primary planet, measured in thousands of kilometers. 5. **Orbital Period (days)**: The time it takes for the satellite to complete one orbit around its primary planet, measured in days. 6. **Orbital Eccentricity**: A measure of how much the orbit deviates from being circular. A value of 0 indicates a perfect circle. 7. **Orbital Inclination**: The tilt of the satellite’s orbit relative to the planet’s equator. **Notes**: - The symbol “~” indicates approximate values. - **Orbital Inclination** is measured relative to the planet’s equator. **Details for Each Planet**: - **Earth**: - Moon: Radius 1738 km, 384.4 x 10^3 km from Earth, 27.32 days orbital period, orbital eccentricity 0.055, inclination 18.3°. - **Mars**: - Phobos: Radius 14 x 12 x 10 km, 9.4 x 10^3 km away, 0.32 days period, 0.018 eccentricity, 1.0° inclination. - Deimos: Radius 8 x 6 x 5 km, 23.5 x 10^3 km away, 1.26 days period, 0.002 eccentricity, 2.8° inclination. - **Jupiter**: - Various satellites such as Amalthea, Io, Europa, Ganymede, Callisto, and Himalia with different radii, distances, periods, eccentricities, and inclinations as listed. - **Saturn**: - Includes Janus, Mimas, Enceladus, Tethys, Dione, Rhea, Titan, Hyperion
Transcribed Image Text:**Table A-11: Principal Satellites of the Solar System** This table provides detailed information on the principal satellites of various planets in the Solar System. It includes data about each satellite's radius, distance from its primary planet, orbital period, orbital eccentricity, and orbital inclination. **Columns**: 1. **Primary**: The planet around which the satellite orbits. 2. **Satellite**: The name of the satellite. 3. **Radius (km)**: The radius of the satellite in kilometers. 4. **Distance from Primary (10^3 km)**: The average distance from the satellite to its primary planet, measured in thousands of kilometers. 5. **Orbital Period (days)**: The time it takes for the satellite to complete one orbit around its primary planet, measured in days. 6. **Orbital Eccentricity**: A measure of how much the orbit deviates from being circular. A value of 0 indicates a perfect circle. 7. **Orbital Inclination**: The tilt of the satellite’s orbit relative to the planet’s equator. **Notes**: - The symbol “~” indicates approximate values. - **Orbital Inclination** is measured relative to the planet’s equator. **Details for Each Planet**: - **Earth**: - Moon: Radius 1738 km, 384.4 x 10^3 km from Earth, 27.32 days orbital period, orbital eccentricity 0.055, inclination 18.3°. - **Mars**: - Phobos: Radius 14 x 12 x 10 km, 9.4 x 10^3 km away, 0.32 days period, 0.018 eccentricity, 1.0° inclination. - Deimos: Radius 8 x 6 x 5 km, 23.5 x 10^3 km away, 1.26 days period, 0.002 eccentricity, 2.8° inclination. - **Jupiter**: - Various satellites such as Amalthea, Io, Europa, Ganymede, Callisto, and Himalia with different radii, distances, periods, eccentricities, and inclinations as listed. - **Saturn**: - Includes Janus, Mimas, Enceladus, Tethys, Dione, Rhea, Titan, Hyperion
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