So now we know it's very red (like kuiper belt objects) and featureless.
Almost certainly not: it's 122° from the ecliptic, so it never even came close to any major body in the solar system.An collision/disturbance within the solar system could still cause it too take that ejection trajectory. Unfortunate we can't take a look, such a missed opportunity!
Can you imagine, if instead of a small rock that was a brown dwarf ejected from a solar system or something.
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An artificial magnetosphere of sufficient size generated at L1 – a point where the gravitational pull of Mars and the sun are at a rough equilibrium — allows Mars to be well protected by what is known as the magnetotail. The L1 point for Mars is about 673,920 miles (or 320 Mars radii) away from the planet. In this image, Green’s team simulated the passage of a hypothetical extreme Interplanetary Coronal Mass Ejection at Mars. By staying inside the magnetotail of the artificial magnetosphere, the Martian atmosphere lost an order of magnitude less material than it would have otherwise. (J. Green)
To quote the first line of a letter published today in the journal Nature, “Every supernova so far observed has been considered to be the terminal explosion of a star.” In other words, when a massive star blows itself up, it should remain dead. This is something astronomers have witnessed thousands of times before with absolutely no exceptions.