Presentation: Venus hot break hypothesis

In summary, a presentation will be given at the Ancient Venus conference in Houston on July 25th. The abstract for the presentation discusses the possibility of a glancing collision between a proto-Mercury and a proto-Venus, which could explain various characteristics of the two bodies such as their slow rotation and different densities. The presenter has previously discussed this theory on a forum two decades ago. Further analysis and calculations are needed to fully explore this idea.
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Andre
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Announcement Venus exchanged rotational energy into heat
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I have thought that a glancing collision between a proto-Mercury and a proto-Venus might explain many characteristics of the two bodies. A glancing collision of two bodies with the same rotation should be expected to cancel some or all of the rotational momentum of both bodies, perhaps explaining the slow rotation of Mercury and Venus. If the collision resulted in transfer of some of the mantle of the proto-Mercury to the proto-Venus this would explain the higher density of Mercury and lower density of Venus. https://nssdc.gsfc.nasa.gov/planetary/factsheet/
Re-accretion of the transferred material to Venus might contribute to its counter rotation.
I do not have the expertise or facilities to do the necessary calculations but perhaps you do.
 

1. What is the Venus hot break hypothesis?

The Venus hot break hypothesis is a scientific theory that suggests Venus may have undergone a catastrophic event in its past that caused a dramatic shift in its climate and atmosphere. This event would have resulted in the extreme heat and pressure that we see on Venus today.

2. How does the Venus hot break hypothesis explain the extreme temperatures on Venus?

The hypothesis proposes that a large amount of carbon dioxide was released into Venus' atmosphere, trapping heat and causing a runaway greenhouse effect. This would have led to the extreme temperatures we see on Venus today, with an average surface temperature of 864 degrees Fahrenheit.

3. What evidence supports the Venus hot break hypothesis?

Scientists have observed a number of features on Venus that support the hot break hypothesis, including the planet's thick atmosphere, lack of water, and high levels of carbon dioxide. Additionally, data from spacecraft missions to Venus have shown evidence of volcanic activity and a young surface, suggesting a recent catastrophic event.

4. Are there any alternative explanations for the extreme temperatures on Venus?

While the Venus hot break hypothesis is the most widely accepted explanation, some scientists have proposed alternative theories. These include a gradual buildup of carbon dioxide over time, or a collision with another object that caused a dramatic increase in temperature. However, these theories do not fully explain all of the observed features on Venus.

5. How does the Venus hot break hypothesis impact our understanding of climate change on Earth?

Studying the Venus hot break hypothesis can provide valuable insights into the potential effects of a runaway greenhouse effect on a planet's climate. By understanding the extreme conditions on Venus, scientists can better understand the potential consequences of increasing carbon dioxide levels on Earth and the importance of mitigating climate change.

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