NASA predicts asteroid to make one of closest approaches to Earth ever recorded
jpl.nasa.gov
jpl.nasa.gov
One problem I like to repeat at times like this, is that these hunts for near earth asteroids look for bright spots that move against the background stars. That's a nice way to find things nearby. But any object on a collision course with earth will not be moving against the background in the days and weeks leading up to the collision when they are also the brightest and most observable. I believe this is why the ones that have exploded in the atmosphere in recent years went completely undetected. It's not just that they're small, but that they don't have the relative motion against the sky to make them stand out.
- Detection in optical by ground-based telescopes is a good technique. You need several exposures and good spot-tracking. Because of the relatively short time-base, you also need good follow-up or else the NEO diverges from your estimated orbit and is lost again!
- The parallax issue you mention comes up more regarding orbit determination than detection per se. (I.e., you need more than just detection to do anything useful.) One link going deep on the relationship of parallax to good orbits: [1]
- There are a bunch of such optical surveys, e.g. Pan-STARRs [3].
- But ground-based telescopes rely on reflected light, and so NEOs coming from certain regions (e.g., within Earth's orbit, but it's worse than that) don't have much reflected sunlight so are hard to detect optically.
- So, IR telescopes can be used, but you have to go above the atmosphere. See, NEOSurveyor [2]. IR is based on the infrared "glow" of a NEO against the background, and so it does not rely on reflected light. So IR telescopes get around many of the geometric limitations of optical.
- What about radar? It's very useful for follow-up orbit determination, but not so good for surveys, because the radar energy diffuses so much. Crudely, if the NEO is R away, you get a 1/R^2 on the way out, and a 1/R^2 on the way back. It's more complicated than that, but this is the reason that radar has limitations for this problem.
[1] https://iopscience.iop.org/article/10.1088/1538-3873/ac43ca/...
[2] https://www.jpl.nasa.gov/missions/near-earth-object-surveyor
My understanding is that the robotic scanning telescopes can detect these objects, but that unless they get a high-quality track, the telescope has already moved on with its scan and the NEO will be lost. That is, detection is hard, but tracking is harder, and you need tracking.
And I guess my comments are also directed at the "systems" aspect of the NEO protection problem - detection, tracking, followup.
> President : Dan, we didn't see this thing coming?
> Dan : Well, our object collison budget's a million dollars, that allows us to track about 3% of the sky, and beg'n your pardon sir, but it's a big-ass sky.
you could put LIGO-type "stationary" satellites around Earth to detect heavy things moving
in boxed grids then estimate trajectory over the affected cubes
"Before encountering Earth, the asteroid’s orbit around the Sun was roughly circular, approximating Earth’s orbit, taking 359 days to complete its orbit about the Sun. After its encounter, the asteroid’s orbit will be more elongated, moving it out to about halfway between Earth’s and Mars’ orbits at its farthest point from the Sun. The asteroid will then complete one orbit every 425 days."
It provides info about those asteroids, as well as any scheduled rocket launches, for any date or date range. And it throws in the moon phase as well.
[1] NeoWs at https://api.nasa.gov/index.html
Discovered 5 days before its closest approach.
It’s amazing how much “stuff” is out there to learn, and how something can sneak in so “close”.
But the other part that I think the original OP is sort of amazed at is that we're unable to detect these through some sort of automated system more accurately. It isn't fair to compare our space/vision capabilities to the eyesight of a person alone. Do we not have satellites or installations doing ""short range"" scanning with radio/laser/something-else-I-am-not-an-astronomer-don't-hate-me ? How come it was an amateur picking this up so close to the specific date?
R-squared is not your friend. This would take a massive amount of energy.
It was about the size golfball/chicken egg held at arms length. I was facing East-South-East (approximately).
It was a bright red, and I could see impact craters on the surface of it. There were no 'flames/fireballs' from orbital entry friction.
The entire incident lasted less then 10 seconds (but this is very much a guess, and impacted by the time-frames involved).
So your asteroid would have to be at least several kilometers across. That approaching dino-killer size. You're definitely misremembering some part of this.
What's the equation to calculate if such object given its mass, velocity, etc would get pulled into Earth orbit or collision or just fly past?
For an incoming object to start orbiting earth, it has to decelerate through active propulsion or aerobraking or something like that.
There is no way for an asteroid and the earth to interact gravitationally to change the asteroid's orbit from what it was coming in. Non-gravitational interactions (like hitting the earth/atmosphere) can do it.
Also, over many interactions and a long time you can have orbital capture in many-body situations, but there is no general equation for this (look up 3 body problem). This is how you get objects accumulating at Lagrange points for example.
TLDR: The equation you're asking for does not exist. Sorry, wrong question!!
It's like that Elisa Wood movie. At least the message got through
I never understood why anyone should give it any more than even a passing thought. As a layman my understanding is that the last great extinction event from an asteroid was like (Wikipedia tells me) 66 million years ago.
With that frequency/odds my fears seem much better afforded toward the dangers of climate change or any number of other issues that likely will have repercussions in my or my grandchildren's lifetimes.
On the scale of things to be concerned about, I'd agree that Climate Change is definitely something that we should be proportionally spending more resource on.
We have the capability of solving multiple problems at once, though - it's not an all-or-nothing thing. So I think running observation/detection systems is worth it, even with the occasional news release about significant close-approaches.
Well said, I agree. This applies to a lot of things that people often ask, “but shouldn’t we focus on X instead?” about.
We have both the people and the resources to do multiple things at once, and we should, if only because it doesn’t help anybody to tell people who’ve spent a large chunk of their lives working on asteroid defense, rockets, crewed spaceflight, etc that their job is gone and they have to start over from scratch and work on X instead.
We've been lucky so far but you'd have to be a fool to rely on luck forever.
Your comment isn't cynical, it is more akin to a lucid perspective of a set of threats.
The economy and threats to democratic process are more worrisome -- and yet at the same time, much more within our capability to fix than an asteroid strike.
For a lucid fictional presentation of an asteroid strike, I recommend "Lucifer's Hammer" by Niven and Pournelle.^1
That sounds very made up.
So the notion was certainly a reasonable one even if not ultimately true.
(And to note: I can't edit my reply now but I read 'there' as 'these'. Obviously there are other (somewhat) cyclic natural catastrophes especially on shorter timescales.)
The Wikipedia article mentions 26 million year intervals. So we're probably good for another 10 million?
[1] https://en.wikipedia.org/wiki/Nemesis_(hypothetical_star)
The current goal of NASA asteroid detection is 90% of 150m asteroids which can cause regional disaster.