(65803) Didymos
Alternative name: Also known as: 1996 GT
Orbital Radius of (65803) Didymos
The (65803) Didymos semi-major axis is a critical orbital parameter that defines the average distance from the Sun. The (65803) Didymos semi-major axis measures 1.64 AU (approximately 2.46e+8 km), which represents the average orbital radius of (65803) Didymos. This measurement is fundamental to understanding (65803) Didymos's position in the Solar System and its relationship with other celestial bodies.
The orbital radius of (65803) Didymos determines how much solar radiation the planet receives, which directly influences its temperature, climate, and overall environmental conditions. This distance places (65803) Didymos in a specific region of the Solar System, each with unique characteristics and scientific significance.
When we examine the (65803) Didymos semi-major axis 1.64 AU, we gain insights into the planet's orbital mechanics, including its orbital period, velocity, and the gravitational forces at play. This parameter is essential for space mission planning and understanding the dynamics of our Solar System.
Mass of (65803) Didymos in kg
The (65803) Didymos mass is a fundamental property that determines many of the planet's physical characteristics. The mass of (65803) Didymos in kg is approximately 5.23e+11 kg, which is 11423106350420.81× less than Earth's mass. This substantial mass creates a significant gravitational field that influences everything from atmospheric retention to orbital dynamics.
Understanding the (65803) Didymos mass allows scientists to calculate other critical properties such as surface gravity, escape velocity, and the planet's ability to retain an atmosphere. The mass also plays a crucial role in determining how (65803) Didymos interacts with other celestial bodies through gravitational forces.
The precise measurement of the mass of (65803) Didymos in kg is essential for space exploration missions, as it affects spacecraft trajectories, landing procedures, and the design of scientific instruments. This fundamental property helps us understand(65803) Didymos's formation history and its place in the evolution of our Solar System.
How Long is a Year on (65803) Didymos?
The (65803) Didymos orbital period defines the length of one complete revolution around the Sun. The (65803) Didymos orbital period is 0.21 hours, which is 40976.10× shorter than Earth's year. This orbital period determines the length of (65803) Didymos's year and directly influences seasonal patterns, climate cycles, and temperature variations.
The (65803) Didymos orbital period is directly related to its distance from the Sun, following Kepler's laws of planetary motion. Planets farther from the Sun have longer orbital periods, while those closer complete their orbits more quickly. This relationship helps explain why (65803) Didymos takes the time it does to complete one full orbit.
Understanding the (65803) Didymos orbital period is crucial for space mission planning, as it affects launch windows, travel times, and the timing of scientific observations. This fundamental orbital parameter also provides insights into the planet's formation history and its current position in the Solar System's dynamic structure.
Distance Between (65803) Didymos and Earth
How far is (65803) Didymos from Earth? This is a question that fascinates both astronomers and space enthusiasts. The distance between (65803) Didymos and Earth varies throughout their orbital cycles, but on average, (65803) Didymos is approximately 9.64e+7 km(0.644 AU) away from Earth. This distance changes as both planets orbit the Sun, with the closest approach (opposition) and farthest separation (conjunction) creating significant variations.
The question "How far is (65803) Didymos from Earth?" has practical implications for space exploration. This distance determines travel time for spacecraft, communication delays for mission control, and the amount of fuel required for interplanetary missions. Understanding this distance is essential for planning future missions to (65803) Didymos.
The distance between (65803) Didymos and Earth is not constant due to the elliptical nature of both planets' orbits. When (65803) Didymos and Earth are on the same side of the Sun (opposition), they are at their closest, making this the optimal time for observations and potential missions. Conversely, when they are on opposite sides of the Sun (conjunction), they are at their farthest separation, which can exceed the average distance significantly.
- Mean Radius
- 0km
- Equatorial Radius
- 0km
- Polar Radius
- 0km
- Mass
- 5.23e+11 kg
- Volume
- 0.00e+0 km³
- Density
- 0g/cm³
- Gravity
- 0m/s²
- Escape Velocity
- 0m/s
- Flattening
- 0
- Average Temperature
- 0.0 K (-273.1 °C)
- Axial Tilt
- 0°
- Semimajor Axis
- 2.46e+8km
- Perihelion
- 1.52e+8km
- Aphelion
- 3.40e+8km
- Eccentricity
- 0.384
- Inclination
- 3.408°
- Sidereal Orbit
- 0.21 hours
- Sidereal Rotation
- 0.00 hours
- Mean Anomaly
- 325.52°
- Argument of Periapsis
- 319.32°
- Longitude of Ascending Node
- 73.193°
Overview of (65803) Didymos
Physical Characteristics
Orbital Properties
Rotation and Tilt
Temperature and Atmosphere
Escape Velocity & Flattening
FAQs About (65803) Didymos
How far is (65803) Didymos from the Sun?
How long is a year on (65803) Didymos?
Does (65803) Didymos have seasons?
- Discovered By
- Spacewatch
- Discovery Date
- 11/04/1996
