No, I'm saying an Earth-life centric metric is a bit of an odd choice when evaluating extrasolar planets.
It's like an African elephant declaring Norway uninhabitable.
No, I'm saying an Earth-life centric metric is a bit of an odd choice when evaluating extrasolar planets.
It's like an African elephant declaring Norway uninhabitable.
We have incontrovertible evidence that water + carbon + time sometimes equals life. We have no evidence of any other non-carbon or non-water chemistries resulting in life so why wouldn't we focus on locations potentially rich in water and carbon first?
Here on Earth, we can barely decide if viruses are life or not, and discover new things within our own bodies pretty regularly, despite... a lot of direct access to them. (Example: https://www.science.org/content/article/it-s-insane-new-viru...)
We should be casting a pretty wide net.
Or maybe we start with what we know (carbon-based), and keep our minds open to other possibilities. Like we do now.
But we know more than one thing. One of those things is the Fermi paradox - that the universe should statistically be full of evidence of life, and yet we struggle to find it. That may be evidence we're making the wrong assumptions.
> keep our minds open to other possibilities...
Yes, and I'd argue that means including scenarios like Jupiter's moons in our search. (As a bonus, Jupiter-style planets, being larger and far from the star, are substantially easier to find.)
We haven't even had the chance to fail yet, the Fermi paradox is not yet in play when we're considering essentially our first move. To extend an analogy from further up thread, it'd be like looking in the Mariana Trench for un-contacted human tribes after taking a quick glance around the neighborhood and deciding there's nothing else to be found anywhere else.
I just think you're confused if you think that observing a specific definition of habitable zone is tantamount to a specific denial of that possibility.