Nereid

Moon
Nereid Radius

Radius of Nereid

The radius of Nereid is one of its most fundamental physical characteristics. The Nereid radius measures approximately 170 km, making it 37.48× smaller than Earth. This measurement represents the average distance from the center of Nereid to its surface, providing crucial information about the celestial body's size and volume.

Understanding the Nereid 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.

Nereid Semi-Major Axis

Orbital Radius of Nereid

The Nereid semi-major axis is a critical orbital parameter that defines the average distance from the Sun. The Nereid semi-major axis measures 0.04 AU (approximately 5.51e+6 km), which represents the average orbital radius of Nereid. This measurement is fundamental to understanding Nereid's position in the Solar System and its relationship with other celestial bodies.

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

When we examine the Nereid semi-major axis 0.04 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.

Nereid Mass

Mass of Nereid in kg

The Nereid mass is a fundamental property that determines many of the planet's physical characteristics. The mass of Nereid in kg is approximately 3.00e+19 kg, which is 199066.67× less than Earth's mass. This substantial mass creates a significant gravitational field that influences everything from atmospheric retention to orbital dynamics.

Understanding the Nereid 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 Nereid interacts with other celestial bodies through gravitational forces.

The precise measurement of the mass of Nereid 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 understandNereid's formation history and its place in the evolution of our Solar System.

Nereid Orbital Period

How Long is a Year on Nereid?

The Nereid orbital period defines the length of one complete revolution around the Sun. The Nereid orbital period is 0.10 hours, which is 87628.38× shorter than Earth's year. This orbital period determines the length of Nereid's year and directly influences seasonal patterns, climate cycles, and temperature variations.

The Nereid 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 Nereid takes the time it does to complete one full orbit.

Understanding the Nereid 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.

How Far is Nereid from Earth?

Distance Between Nereid and Earth

How far is Nereid from Earth? This is a question that fascinates both astronomers and space enthusiasts. The distance between Nereid and Earth varies throughout their orbital cycles, but on average, Nereid is approximately 1.44e+8 km(0.963 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 Nereid 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 Nereid.

The distance between Nereid and Earth is not constant due to the elliptical nature of both planets' orbits. When Nereid 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
170km
Equatorial Radius
170km
Polar Radius
0km
Mass
3.00e+19 kg
Volume
2.05e+7 km³
Density
1.5g/cm³
Gravity
0.071m/s²
Escape Velocity
0m/s
Flattening
0
Average Temperature
0.0 K (-273.1 °C)
Axial Tilt
0°
Semimajor Axis
5.51e+6km
Perihelion
1.37e+6km
Aphelion
9.66e+6km
Eccentricity
0.751
Inclination
7.23°
Sidereal Orbit
0.10 hours
Sidereal Rotation
0 seconds
Mean Anomaly
0°
Argument of Periapsis
0°
Longitude of Ascending Node
0°

Overview of Nereid

Nereid is a fascinating moon in our Solar System that has captured the attention of astronomers and space enthusiasts alike. With a Nereid radius of 170 km, making it 37.5× 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 5.51e+6 km (0.037 AU) from the Sun, Nereid occupies a significant place in the Solar System's architecture. As a moon, Nereid demonstrates the incredible diversity of natural satellites that orbit larger celestial bodies throughout our Solar System.

Physical Characteristics

The Nereid physical characteristics reveal a world of remarkable dimensions and properties. The Nereid radius measures 170 km, making it 37.5× smaller than Earth's size. The Nereid mass of 3.00e+19 kg represents 199066.7× smaller than Earth's mass, giving this world substantial gravitational influence. With a volume of 2.05e+7 km³, Nereid occupies significant space in the Solar System. The Nereid density of 1.5 g/cm³ (3.7× smaller than Earth's density) provides clues about its internal composition, while the surface gravity of 0.071 m/s² (138.2× smaller than Earth's gravity) determines how objects behave on its surface. The low density indicates a composition dominated by lighter elements, characteristic of gas giants or icy bodies.

Orbital Properties

The Nereid orbit reveals fascinating details about its journey around the Sun and its relationship to other Solar System objects. The Nereid orbit has a semimajor axis of 5.51e+6 km (0.037 AU), placing it 27.1× smaller than Earth's distance from the Sun. At its closest approach (perihelion), Nereid comes within 1.37e+6 km of the Sun, while at its farthest point (aphelion), it reaches 9.66e+6 km, creating a 150.2% variation in solar distance. The Nereid orbit is highly elliptical with an eccentricity of 0.751 (45.0× Earth's orbital eccentricity), leading to extreme variations in temperature and solar exposure. The Nereid orbit takes 0.10 hours to complete (87628.4× smaller than Earth's orbital period), defining the length of its year. The orbital inclination of 7.23° indicates how much the Nereid orbit is tilted relative to the Solar System's ecliptic plane. This moderate inclination indicates a typical orbital evolution for objects in this region of the Solar System.

Rotation and Tilt

The Nereid rotation and axial orientation provide crucial insights into its daily and seasonal cycles, as well as its orbital dynamics. The Nereid axial tilt of 0° determines the intensity and nature of seasonal variations. With minimal axial tilt, Nereid experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year. The orbital orientation parameters reveal additional details about Nereid'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 Nereid temperature and atmospheric conditions are fundamental to understanding its habitability and environmental characteristics. The Nereid average temperature of 0.0 K (-273.1 °C) (-459.7°F) provides the baseline for understanding its climate. These extremely cold temperatures make Nereid 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), Nereid presents a dramatically different thermal environment. Being closer to the Sun than Earth, Nereid receives more intense solar radiation, contributing to its temperature profile. The elliptical orbit creates significant temperature variations throughout the year, with extreme seasonal changes.

Escape Velocity & Flattening

The Nereid escape velocity and shape characteristics reveal important details about its gravitational field and rotational dynamics. The Nereid 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 Nereid to retain a substantial atmosphere. The Nereid 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 Nereid

What is the gravity on Nereid?

The gravity on Nereid is 0.071 m/s² (138.2× smaller than Earth's gravity). This gravitational force determines how objects behave on the surface, affects atmospheric retention, and influences the planet's ability to hold onto gases and particles. A person weighing 70 kg on Earth would weigh 0.5 kg on Nereid.

How big is Nereid compared to Earth?

Nereid has a radius of 170 km, making it 37.5× smaller than Earth's size. In terms of volume, Nereid 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 Nereid from the Sun?

Nereid orbits at an average distance of 5.51e+6 km (0.037 AU) from the Sun, placing it 27.1× 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.

How long is a year on Nereid?

A year on Nereid lasts 0.10 hours (87628.4× smaller than Earth's orbital period). This orbital period defines the length of the planet's year and affects seasonal patterns, temperature variations, and the overall climate cycle.

What is Nereid made of?

Nereid has a density of 1.5 g/cm³ (3.7× smaller than Earth's density). This density provides important clues about the planet's internal composition. The low density indicates a composition dominated by lighter elements, characteristic of gas giants or icy bodies.

Does Nereid have seasons?

Nereid 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
Gerard Kuiper
Discovery Date
01/05/1949
Raw Data