762 Pulcova

762 Pulcova is a fascinating asteroid in our Solar System that has captured the attention of astronomers and space enthusiasts alike. With a 762 Pulcova radius of 78.6 km, making it 81.1× 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 4.73e+8 km (3.159 AU) from the Sun, 762 Pulcova occupies a significant place in the Solar System's architecture. As an asteroid, 762 Pulcova represents the remnants of the early Solar System, providing valuable insights into the formation and evolution of our cosmic neighborhood.

The 762 Pulcova physical characteristics reveal a world of remarkable dimensions and properties. The 762 Pulcova radius measures 78.6 km, making it 81.1× smaller than Earth's size. The 762 Pulcova mass of 2.60e+18 kg represents 2296923.1× smaller than Earth's mass, giving this world substantial gravitational influence.

The 762 Pulcova orbit reveals fascinating details about its journey around the Sun and its relationship to other Solar System objects. The 762 Pulcova orbit has a semimajor axis of 4.73e+8 km (3.159 AU), placing it 3.2× Earth's distance from the Sun. At its closest approach (perihelion), 762 Pulcova comes within 4.27e+8 km of the Sun, while at its farthest point (aphelion), it reaches 5.18e+8 km, creating a 19.1% variation in solar distance. The 762 Pulcova orbit is nearly circular with an eccentricity of 0.096 (5.7× Earth's orbital eccentricity), resulting in relatively stable solar heating throughout its year. The 762 Pulcova orbit takes 0.57 hours to complete (15398.2× smaller than Earth's orbital period), defining the length of its year. The orbital inclination of 13.049° indicates how much the 762 Pulcova 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 762 Pulcova rotation and axial orientation provide crucial insights into its daily and seasonal cycles, as well as its orbital dynamics. The 762 Pulcova axial tilt of 0° determines the intensity and nature of seasonal variations. With minimal axial tilt, 762 Pulcova experiences virtually no seasonal changes, maintaining relatively constant temperatures throughout its year. The orbital orientation parameters reveal additional details about 762 Pulcova's position in space. The mean anomaly of 0° indicates the planet's current position in its orbit relative to its perihelion. The argument of periapsis of 0° shows how the orbit's orientation changes over time due to gravitational perturbations. The longitude of ascending node of 0° defines the reference point where the orbit crosses the ecliptic plane.

The 762 Pulcova temperature and atmospheric conditions are fundamental to understanding its habitability and environmental characteristics. The 762 Pulcova average temperature of 0.0 K (-273.1 °C) (-459.7°F) provides the baseline for understanding its climate. These extremely cold temperatures make 762 Pulcova 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), 762 Pulcova presents a dramatically different thermal environment. Being farther from the Sun than Earth, 762 Pulcova receives less solar radiation, resulting in cooler conditions.

The 762 Pulcova escape velocity and shape characteristics reveal important details about its gravitational field and rotational dynamics. The 762 Pulcova 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 762 Pulcova to retain a substantial atmosphere. The 762 Pulcova 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.