Xiangliu

Moon
Xiangliu Radius

Radius of Xiangliu

The radius of Xiangliu is one of its most fundamental physical characteristics. The Xiangliu radius measures approximately 150 km, making it 42.47× smaller than Earth. This measurement represents the average distance from the center of Xiangliu to its surface, providing crucial information about the celestial body's size and volume.

Understanding the Xiangliu radius is essential for calculating other important properties such as surface area, volume, and gravitational characteristics. The radius directly influences how we perceive and study this fascinating object in our Solar System.

Xiangliu Semi-Major Axis

Orbital Radius of Xiangliu

The Xiangliu semi-major axis is a critical orbital parameter that defines the average distance from the Sun. The Xiangliu semi-major axis measures 0.00 AU (approximately 15,000 km), which represents the average orbital radius of Xiangliu. This measurement is fundamental to understanding Xiangliu's position in the Solar System and its relationship with other celestial bodies.

The orbital radius of Xiangliu determines how much solar radiation the planet receives, which directly influences its temperature, climate, and overall environmental conditions. This distance places Xiangliu in a specific region of the Solar System, each with unique characteristics and scientific significance.

When we examine the Xiangliu semi-major axis 0.00 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.

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How Far is Xiangliu from Earth?

Distance Between Xiangliu and Earth

How far is Xiangliu from Earth? This is a question that fascinates both astronomers and space enthusiasts. The distance between Xiangliu and Earth varies throughout their orbital cycles, but on average, Xiangliu is approximately 1.50e+8 km(1.000 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 Xiangliu 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 Xiangliu.

The distance between Xiangliu and Earth is not constant due to the elliptical nature of both planets' orbits. When Xiangliu 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.

Physical Properties
Mean Radius
0km
Equatorial Radius
150km
Polar Radius
0km
Mass
Volume
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
15,000km
Perihelion
0km
Aphelion
0km
Eccentricity
0
Inclination
0°
Sidereal Orbit
0 seconds
Sidereal Rotation
0 seconds
Mean Anomaly
0°
Argument of Periapsis
0°
Longitude of Ascending Node
0°

Overview of Xiangliu

Xiangliu is a fascinating moon in our Solar System that has captured the attention of astronomers and space enthusiasts alike. With a Xiangliu radius of 150 km, making it 42.5× smaller than Earth's size, this celestial body presents unique characteristics that distinguish it from other objects in our cosmic neighborhood. Positioned at an average distance of 15,000 km (0.000 AU) from the Sun, Xiangliu occupies a significant place in the Solar System's architecture. As a moon, Xiangliu demonstrates the incredible diversity of natural satellites that orbit larger celestial bodies throughout our Solar System.

Physical Characteristics

The Xiangliu physical characteristics reveal a world of remarkable dimensions and properties. The Xiangliu radius measures 150 km, making it 42.5× smaller than Earth's size.

Orbital Properties

The Xiangliu orbit reveals fascinating details about its journey around the Sun and its relationship to other Solar System objects. The Xiangliu orbit has a semimajor axis of 15,000 km (0.000 AU), placing it 9973.2× smaller than Earth's distance from the Sun. The Xiangliu orbit is nearly circular with an eccentricity of 0, resulting in relatively stable solar heating throughout its year. The orbital inclination of indicates how much the Xiangliu orbit is tilted relative to the Solar System's ecliptic plane. This low inclination means Xiangliu follows a path very close to the plane where most planets orbit, suggesting a stable formation history.

Rotation and Tilt

The Xiangliu rotation and axial orientation provide crucial insights into its daily and seasonal cycles, as well as its orbital dynamics. The Xiangliu axial tilt of 0° determines the intensity and nature of seasonal variations. With minimal axial tilt, Xiangliu experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year. The orbital orientation parameters reveal additional details about Xiangliu's position in space. The mean anomaly of indicates the planet's current position in its orbit relative to its perihelion. The argument of periapsis of shows how the orbit's orientation changes over time due to gravitational perturbations. The longitude of ascending node of defines the reference point where the orbit crosses the ecliptic plane.

Temperature and Atmosphere

The Xiangliu temperature and atmospheric conditions are fundamental to understanding its habitability and environmental characteristics. The Xiangliu average temperature of 0.0 K (-273.1 °C) (-459.7°F) provides the baseline for understanding its climate. These extremely cold temperatures make Xiangliu inhospitable to life as we know it, with any atmosphere likely frozen solid on the surface. Compared to Earth's average temperature of 15°C (59°F), Xiangliu presents a dramatically different thermal environment. Being closer to the Sun than Earth, Xiangliu receives more intense solar radiation, contributing to its temperature profile.

Escape Velocity & Flattening

The Xiangliu escape velocity and shape characteristics reveal important details about its gravitational field and rotational dynamics. The Xiangliu escape velocity of 0 m/s determines how easily objects can break free from its gravitational pull. This relatively low escape velocity means that gases and light molecules can easily escape into space, making it difficult for Xiangliu to retain a substantial atmosphere. The Xiangliu flattening of 0.0000% indicates how much the planet's rotation affects its shape. This minimal flattening suggests a nearly spherical shape, indicating either slow rotation or a very rigid internal structure.

FAQs About Xiangliu

How big is Xiangliu compared to Earth?

Xiangliu has a radius of 150 km, making it 42.5× smaller than Earth's size. In terms of volume, Xiangliu is 0.0× the size of Earth. This size difference significantly impacts the planet's gravity, atmospheric retention, geological processes, and overall planetary characteristics.

How far is Xiangliu from the Sun?

Xiangliu orbits at an average distance of 15,000 km (0.000 AU) from the Sun, placing it 9973.2× smaller than Earth's distance from the Sun. This distance determines the amount of solar radiation the planet receives and significantly influences its temperature and climate.

Does Xiangliu have seasons?

Xiangliu has an axial tilt of . With minimal axial tilt, the planet experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year.
Discovery Information
Discovered By
Gábor Marton, Csaba Kiss et Thomas Müller
Discovery Date
17/10/2016
Raw Data