Do you have anything to say about the science?
I had to think of the novel "Big planet" by Jack Vance when reading this.
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A) This article displays insufficient understanding of geometry - twice the diameter makes for eight times the size, I believe.
B) I don't know why no one seems to consider the that difference in light pressure between an inner stellar system and the outer parts around a new star may make a huge difference in the amount of gas available for protoplanets to accrete as they form.
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More bad math. Must've been a screw-up in the press release...
Also, 3 billion years is plenty of time for heavier elements to form - you just know the very first generation of stars were ungodly huge, many with lifespans easily in the hundred of millions of years.
A) This article displays insufficient understanding of geometry - twice the diameter makes for eight times the size, I believe.
B) I don't know why no one seems to consider the that difference in light pressure between an inner stellar system and the outer parts around a new star may make a huge difference in the amount of gas available for protoplanets to accrete as they form.
More bad math. Must've been a screw-up in the press release...[/quote]
Also, 3 billion years is plenty of time for heavier elements to form - you just know the very first generation of stars were ungodly huge, many with lifespans easily in the hundred of millions of years.
Well both, being very closely related concepts. I'm not sure there's any significant distinction in this context. The planet is far more than twice as big in three dimensions.A) This article displays insufficient understanding of geometry - twice the diameter makes for eight times the size, I believe.
B) I don't know why no one seems to consider the that difference in light pressure between an inner stellar system and the outer parts around a new star may make a huge difference in the amount of gas available for protoplanets to accrete as they form.
A) size, or volume? Don't know if this has the same meaning in English as in Dutch.
B) technically, protoplanets accrete by taking in 'dust'. The 'gaseous' stuff becomes atmosphere. Less 'dust' is available the further you go out from a (proto)star, or more precise, its less concentrated.And the gaseous particles are lighter and more effected by light pressure. Pretty intuitive, and we're talking about very close-in orbits.
Which only underlines my point even more. I was being conservative without bothering to look it up.More bad math. Must've been a screw-up in the press release...
Also, 3 billion years is plenty of time for heavier elements to form - you just know the very first generation of stars were ungodly huge, many with lifespans easily in the hundred of millions of years.
Those ungodly huge stars (hundreds of solar masses) barely had time to form before reaching End Of Life, and had a lifespan of only a few million years, not hundreds.