Maybe galactic risks like these are part of the Great Filter.
Maybe galactic risks like these are part of the Great Filter.
Worrying about it is like stressing out over what you are going to name your super-yacht, when you're broke, unemployed, homeless, and are dying of lung cancer. It's the most absurdly pointless form of bikeshedding. There are plenty of immediate and catastrophic disasters that we should be preparing for, first.
https://spaceguardcentre.com/asteroids-deflected-with-paint/
Asteroids that hit Earth are in near-Earth orbits. For a first intercept event the odds of an asteroid just happening to hit an Earth sized target as opposed to, say, a 1000x Earth sized "near miss" target is incredibly unlikely. We get a few near-miss events of a given asteroid before an impact happens.
The asteroid that wiped out the dinosaurs was between 3 and 10 miles diameter. 2014 UN271 is 100km-370km.
Would we have discovered 2014 UN271 earlier had its orbit brought it closer to Earth? It’s making its closest approach in 2031 (ok, 11AU away!), only 17 years after discovery.
And sure, incredibly unlikely something that size would hit Earth, but just an example of something that is very large, and discovered shortly before it makes its closest approach.
My understanding is that this kind of threat is usually lumped in with comets, whereas threat asteroids are lumped in with low eccentricity big rocks.
Comets, though. We keep spotting alarmingly large comets only when they get close enough to the sun to show up in low-sensitivity sky surveys, long after they've crossed the Earth's orbit. https://en.wikipedia.org/wiki/C/2020_F8_(SWAN)
A ultra-high eccentricity Oort object, covered with low-albedo goop from spending millions of years in the periphery of the solar system is going to be damn hard to detect. Worse yet, they'll be traveling fast. Kinetic energy is the square of velocity. Won't ever see em coming, and they'll hit hard. Worst of all worlds.
Radar is tempting, but the tyranny of the inverse square law limits its use. (Worse-- the pulse has to make it out to the object, and then be reflected back. Inverse fourth power!) All those great radar images of asteroids made by Arecibo were done during their closest approach to Earth. This[1] claims its useful range was "~2 lunar distances". This was with a 305 meter dish and 1 MW of transmit power! Also, Arecibo collapsed, and nobody seems to be in a hurry to build a replacement. (The 500 meter dish in China doesn't have a transmitter)
Assuming you have infinite power, (With a moon-based dish, maybe, otherwise your gigawatts of power just ionize the air in front of the feed horn) you have other practical problems. Bigger the dish, better the gain, narrower the beam width. Arecibo had a 2 arcminute beam. 60 arcminutes to the degree: 21,600 arcminutes to a full circle. Assuming you're surveying out to Jupiter's orbit, 43 minutes for the pulse to get out there, 43 minutes back: 645 days to survey a strip 2 arcminutes wide and 360 degrees long. Which... wouldn't have caught C/2020 F8 (SWAN), which came in 110 degrees off the ecliptic. Surveying the entire night sky would take 6,074.9 years. Just out to Jupiter! You're not even looking into the cloud of outer objects, just spotting infalling ones.
1: https://www.hou.usra.edu/meetings/orbitaldebris2019/orbital2...
there's no concept of money and cost left if humanity goes extinct ... so it can't be "expensive".