Lizard-Planets Wiki

Lizard-718-O

Lizard-718-O

Lizard-718-O
Astrographical Info
Age1.2 Billion Years
Axial Tilt31°
ClassTerrestrial Exoplanet
Diameter22,358 km
Gravity1.79 g
Mass6.564 Earths
Suns3
Orbital
GalaxyAbsthaca Galaxy (formerly) Elkska Galaxy
Orbital Period0.6441 Years
Rotation Period4.509 Days
Semimajor Axis0.5 AU
Solar Day4.509 (1:1) Days
SystemLizard-718
Atmosphere
Atmospheric ColorYellow
Atmospheric CompositionCO₂, SO₂, CH₄
Atmospheric ToxicityDeath in 2 Seconds
Atmospheric Pressure133 atm
Greenhouse Eff777°C
Temperature3177°C (5750.6°F)
Surface
Major MoonsPagiogawa, Niunope
Moons2
Sea CompositionFe
TerrainHellish Wasteland
Water StateWater Decomposes
Other
Affiliations
Bow Shock Distance78,000 km
ClimateSuperheated lava hellscape
GovernmentNot Present
Other NotesHot enough to boil steel
Primary Core ElementFe, Ni
Strength57 µT
Tail LengthPossibly 7,040,000 km

Description

Planet Lizard-718-O is a scorching, Venus-like terrestrial planet located within the Lizard star cluster. With a diameter of 22,358 km and a mass 6.5629 times that of Earth, it is characterized by extreme geothermal activity. The surface is dominated by vast liquid magma oceans, extensive basalt deltas, and expansive lava plains crisscrossed by glowing rivers of molten rock. The planet's atmosphere is thick and composed primarily of carbon dioxide, sulfur dioxide, and trace amounts of helium, contributing to a runaway greenhouse effect. Surface temperatures exceed 1,200°C, preventing the formation of stable solid landmasses in many regions. Despite its hellish conditions, Lizard-718-O boasts two moons, Pagiogawa and Niunope, with Niunope hosting a ring system and signs of life.

History

Lizard-718-O formed approximately 1.2 billion years ago during the early stages of the Lizard star cluster's development. Intense gravitational interactions with nearby planetary bodies likely contributed to its prolonged geological instability. Over time, tidal heating from its moons, particularly Niunope, exacerbated its volcanic nature, creating a surface dominated by tectonic upheaval. The Lizards first observed the planet in 9456 using advanced telescopes orbiting Lizard-953-E. In 9498, a probe mission known as 'Vulkara-I' was launched to study its geology and the mysterious rings around Niunope. The mission revealed unique metal-rich minerals within the basalt plains, sparking interest in potential industrial applications.

Habitat

While Lizard-718-O itself is inhospitable to life as we know it, its moon Niunope presents a remarkable contrast. Orbiting with a faint but dense ring system composed of ice, rock, and metal debris, Niunope harbors microbial life in its subsurface oceans. These extremophiles thrive in the heated liquid water beneath an icy crust, sustained by hydrothermal vents and tidal forces. The Lizards have established several observation satellites around Niunope to monitor biological activity, with ongoing studies hinting at the potential for more complex life forms.

Extras

  • Moons:
    • Pagiogawa: A small, rocky moon with a heavily cratered surface, lacking an atmosphere.
    • Niunope: The larger of the two moons, boasting a ring system and multicellular life.
  • Tidal Locking: Lizard-718-O is partially tidally locked with its star, resulting in one hemisphere experiencing continuous daylight.
  • Mineral Wealth: The basalt plains contain significant deposits of rare metals, including osmium and iridium, offering potential economic value.
  • Scientific Importance: Lizard-718-O is studied to better understand planetary formation, geothermal dynamics, and the potential for life on moons orbiting hostile planets.