Spectroscopic analysis of the exoplanet K2-315b has confirmed the concurrent presence of both atmospheric methane and water vapor. According to atmospheric circulation models, whenever an exoplanet contains both methane and water vapor in its atmosphere, high-altitude silicate cloud decks inevitably form. Furthermore, such silicate cloud decks can form only if the planet's equilibrium temperature remains below and its upper-atmosphere wind speeds exceed . Finally, all exoplanets with equilibrium temperatures below undergo significant atmospheric hydrogen retention.
If the statements above are true, which of the following must also be true regarding K2-315b?
- AHigh-altitude silicate cloud decks can form on an exoplanet only if both atmospheric methane and water vapor are present.
- BAny exoplanet with upper-atmosphere wind speeds exceeding will undergo atmospheric hydrogen retention.
- K2-315b undergoes significant atmospheric hydrogen retention.Answer
- DK2-315b's equilibrium temperature is greater than or equal to .
- EThe presence of water vapor on K2-315b is the primary cause of its high upper-atmosphere wind speeds.
Answer
K2-315b undergoes significant atmospheric hydrogen retention.
The passage establishes a chain of formal conditions. First, K2-315b has both methane and water vapor. Second, whenever both gases are present, silicate cloud decks form. Therefore, K2-315b has silicate cloud decks. Third, silicate cloud decks can form only if the equilibrium temperature is below . Since cloud decks exist on K2-315b, its temperature must be below . Fourth, any planet with a temperature below undergoes atmospheric hydrogen retention. Consequently, it must be true that K2-315b undergoes significant atmospheric hydrogen retention.
Step-by-Step Solution
Key Concept
Conditional logic chains and contrapositives
Estimated Time:2m 0s