Mission

VERITAS

NASA Venus orbiter to map the planet's surface through its clouds and learn how Venus and Earth came to differ.

VERITAS is a NASA mission to orbit Venus and map its surface, to reveal how the paths of Venus and Earth diverged.[1] The name stands for Venus Emissivity, Radio Science, InSAR, Topography and Spectroscopy, and veritas means truth in Latin.[1] The mission is led by NASA's Jet Propulsion Laboratory.[1]

The mission

VERITAS is a solar-powered orbiter. After arriving at Venus, it is to use aerobraking, dipping into the upper atmosphere to slow down and reshape its orbit, before settling into a near-polar orbit about 400 km above the surface.[1] From there it is to make maps far more detailed than those of NASA's Magellan mission, which mapped Venus by radar.[1]

The mission is to look for answers to fundamental questions: whether Venus has continents like Earth's that formed in the presence of water, whether its volcanism is continuous or comes and goes, and whether the planet has plate tectonics.[1] It is also to make the first maps of regions where geologic processes are actively changing the surface.[1]

Why Venus

Venus is similar to Earth in structure and size, but its thick atmosphere traps heat in a runaway greenhouse effect, making it the hottest planet in the solar system.[1] Together with DAVINCI, VERITAS is to be the first NASA mission to Venus since the 1990s.[1][2]

Milestones

  1. In 2031 expected
    Launch

Dates marked expected are agency estimates.

All missions and what each does next

Sources

  1. [1]NASA, VERITAS — science.nasa.gov, retrieved October 26, 2026
  2. [2]NASA, DAVINCI — science.nasa.gov, retrieved October 26, 2026

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