- #1
DaveC426913
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- TL;DR Summary
- With all the exoplanets we've confirmed, can we extrapolate to predict Earth-twins?
Each new report of a confirmed exoplanet adds to the database of knowledge. For obvious reasons, our confirmations seem to stack up in the areas we are currently best able to detect. eg.:
Large bodies: Jupiter-sized down to Sub-Neptune-sized, with a smattering of super-Earths.
Nape-of-star bodies that orbit extremely close.
I presume our dataset finds lots of these because of our detection methods. The implication is that our detection methods are still too rough to find a good cross-section of Earth-twins. It does not mean they not there to be found.
But are we reaching a point where we can start to apply some numbers to our blind spots?
Can we predict with any confidence how many Earth-sized bodies we are likely to find in the Goldilocks Zone and yet still be distant enough (meaning a sunlike star) to dodge the exigencies of tidal-locking?
Large bodies: Jupiter-sized down to Sub-Neptune-sized, with a smattering of super-Earths.
Nape-of-star bodies that orbit extremely close.
I presume our dataset finds lots of these because of our detection methods. The implication is that our detection methods are still too rough to find a good cross-section of Earth-twins. It does not mean they not there to be found.
But are we reaching a point where we can start to apply some numbers to our blind spots?
Can we predict with any confidence how many Earth-sized bodies we are likely to find in the Goldilocks Zone and yet still be distant enough (meaning a sunlike star) to dodge the exigencies of tidal-locking?