Talk:Venus
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![]() | On 24 August 2023, it was proposed that this article be moved from Venus to Venus (planet). The result of the discussion was Not moved. |
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Presence of Phosphine on Venus
[edit]The statement "By late October 2020, re-analysis of data with a proper subtraction of background did not result in the detection of phosphine" seems to have now itself been rendered outdated by the original team[1] who has now found a smaller amount of phosphine but still seems to have found phosphine none the less. Maybe amending this section to say the status of phosphine is still uncertain considering the multiple contradictory analyses of the atmosphere are now available. — Preceding unsigned comment added by Dmesco17 (talk • contribs)
References
- ^ Greaves, Jane. "Re-analysis of Phosphine in Venus' Clouds". arXiv. Retrieved 16 Nov 2020.
Clarification on atmospheric influence on Venus' rotation
[edit]Hello, I would like to point out a possible innacuracy in the introduction, paragraph 2:
“The rotation of Venus has been slowed and turned against its orbital direction (retrograde) by the currents and drag of its atmosphere.”
After reviewing the cited source [23] "Atmospheric dynamics of a near tidally locked Earth-sized planet" (Nature Astronomy, 2022), it appears that the paper discusses atmospheric torque influencing Venus' rotation rate, but does not state that the atmosphere reversed the planet’s spin direction.
To my knowledge, current scientific consensus attributes the retrograde rotation to a combination of early impacts, tidal interactions, and possibly atmospheric effects — but not atmospheric drag alone.
I would like to propose the following revision for improved accuracy:
“Venus' rotation has been influenced by the drag of its dense atmosphere, which slows its rotation and prevents tidal locking with the Sun. The planet's retrograde rotation is thought to result from a combination of atmospheric dynamics, tidal interactions, and early impacts.”
Reference: The four final rotation states of Venus
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