136108 Haumea

136108 Haumea is a fascinating dwarf planet in our Solar System that has captured the attention of astronomers and space enthusiasts alike. Positioned at an average distance of 6.43e+9 km (42.995 AU) from the Sun, 136108 Haumea occupies a significant place in the Solar System's architecture.

The 136108 Haumea physical characteristics reveal a world of remarkable dimensions and properties. The 136108 Haumea mass of 4.01e+21 kg represents 1490.8× smaller than Earth's mass, giving this world substantial gravitational influence. With a volume of 2.40e+9 km³, 136108 Haumea occupies significant space in the Solar System. The 136108 Haumea density of 2.6 g/cm³ (2.1× smaller than Earth's density) provides clues about its internal composition, while the surface gravity of 0.401 m/s² (24.5× smaller than Earth's gravity) determines how objects behave on its surface. The moderate density suggests a mixed composition of rocky and icy materials.

The 136108 Haumea orbit reveals fascinating details about its journey around the Sun and its relationship to other Solar System objects. The 136108 Haumea orbit has a semimajor axis of 6.43e+9 km (42.995 AU), placing it 43.0× Earth's distance from the Sun. At its closest approach (perihelion), 136108 Haumea comes within 5.16e+9 km of the Sun, while at its farthest point (aphelion), it reaches 7.71e+9 km, creating a 39.6% variation in solar distance. The 136108 Haumea orbit is moderately elliptical with an eccentricity of 0.191 (11.5× Earth's orbital eccentricity), creating noticeable seasonal variations in solar radiation. The 136108 Haumea orbit takes 1.20 days to complete (304.1× smaller than Earth's orbital period), defining the length of its year. The orbital inclination of 28.19° indicates how much the 136108 Haumea 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.

The 136108 Haumea rotation and axial orientation provide crucial insights into its daily and seasonal cycles, as well as its orbital dynamics. The 136108 Haumea rotation period of 0.00 hours (21980.6× smaller than Earth's rotation period) determines the length of its day. This extremely fast rotation creates intense centrifugal forces and may contribute to the planet's flattened shape. The 136108 Haumea axial tilt of 0° determines the intensity and nature of seasonal variations. With minimal axial tilt, 136108 Haumea experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year. The orbital orientation parameters reveal additional details about 136108 Haumea's position in space. The mean anomaly of 218.205° indicates the planet's current position in its orbit relative to its perihelion. The argument of periapsis of 239.041° shows how the orbit's orientation changes over time due to gravitational perturbations. The longitude of ascending node of 122.167° defines the reference point where the orbit crosses the ecliptic plane.

The 136108 Haumea temperature and atmospheric conditions are fundamental to understanding its habitability and environmental characteristics. The 136108 Haumea average temperature of 50.0 K (-223.1 °C) (-369.7°F) provides the baseline for understanding its climate. These extremely cold temperatures make 136108 Haumea 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), 136108 Haumea presents a dramatically different thermal environment. Being farther from the Sun than Earth, 136108 Haumea receives less solar radiation, resulting in cooler conditions. The elliptical orbit creates significant temperature variations throughout the year, with extreme seasonal changes.

The 136108 Haumea escape velocity and shape characteristics reveal important details about its gravitational field and rotational dynamics. The 136108 Haumea escape velocity of 809 m/s (13.8× smaller than Earth's escape velocity) 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 136108 Haumea to retain a substantial atmosphere. The 136108 Haumea flattening of 61.0200% indicates how much the planet's rotation affects its shape. This significant flattening indicates rapid rotation that has substantially deformed the planet's shape, creating a pronounced equatorial bulge.