It looks like you're using an Ad Blocker.
Please white-list or disable AboveTopSecret.com in your ad-blocking tool.
Thank you.
Some features of ATS will be disabled while you continue to use an ad-blocker.
originally posted by: Phage
a reply to: willzilla
That's sort of part of the problem of figuring out what the heck it is. Other studies have concluded that there must be a lot of those things out there so how could such an odd thing be relatively common? This provides an answer.
At the same time, it also provides an explanation for why the surface of the object is so "dry", and how getting close to the Sun could cause volatile materials (H2O) beneath the surface to be ejected and produce that famous non-gravitational acceleration.
It's a nice neat package.
But I have never said that `Oumuamua is not a spaceship.
close enough to become malleable but strong enough to not be ripped apart by tidal gravity forces
The tidal fragmentation scenario, as Zhang and Lin call it, provides an elegant solution backed by computer models that simulated the structural dynamics of a parent object as it strayed too close to its host star. As the models showed, a parent object like a planetesimal (an embryonic planet) or even a terrestrial, Earth-like planet, that ventures to within a few hundred thousand kilometers of its host star will start to distort—and distort very badly.
The process is akin to making a super-thin snake from a ball of Play-Doh. As the Play-Doh gets progressively thinner, smaller chunks start to shred off, with each of the bits still retaining their elongated shape.
In the case of ‘Oumuamua and other nascent interstellar objects, the hot, elongated fragments are quite malleable, consisting of a jumble of tiny pieces. As this loose collection of material ventures farther away from its host star, the bits rapidly start to cool and congeal to one another, forming a crust that defines the ultimate shape and structural integrity of the object. The ratio of the long axis to the short axis can be as much as 10:1, according to the computer models.
originally posted by: St Udio
perhaps the very long, thin object is a orphaned structural metal component of a destroyed Dyson Sphere
thrown into Galactic Space by the exploding Star it once enveloped
~~ Ergo, just a glimpse of Galactic flotsam, which the Milky Way might be cluttered with ~~
SEE: Dyson sphere - Wikipedia
en.wikipedia.org...
A Dyson sphere is a hypothetical megastructure that completely encompasses a star and captures a large percentage of its power output. The concept is a thought experiment that attempts to explain how a spacefaring civilization would meet its energy requirements once those requirements exceed what can be generated from the home planet's resources alone...
more: www.bing.com... 4581a467941f83f5efb7