Hopefully NASA got some good off-axis shots of the pair as Lucy approached and departed to determine the spacing. It's hard to tell from the image above if they're right on top of each other or well spread.
I would assume it's tidally locked. I hope they got enough data to estimate the orbital period. That would let them calculate the mass of the larger part.View attachment 66662
Is it me or does it look tidally locked?
(I'm not sure why the gif from NASA had a transparent frame around it)
I doubt you're seeing any of the orbit. Lucy was whizzing past. So its view changed as it went, but the two bodies were essentially in the same orientation as when they started. Without doing some back-of-the-envelope math, I would expect the period to be many hours.View attachment 66662
Is it me or does it look tidally locked?
(I'm not sure why the gif from NASA had a transparent frame around it)
Behbeh! That's a behbeh asteroid!That's no moon..... It's a baby.
What's with the bulge around the midpoint of both of these rocks and Bennu? Seems to be a common thread amongst the few small asteroids we've recently seen.
Last year's thanksgiving dinner? That's my excuse anyway.
“That log had a child!”That's no moon..... It's a baby.
Given the name of the instrument (L-LORRI), is it fair to assume that this is a descendant of the LORRI that New Horizons used?
"Dinki" being the smaller one, of course!I hope they devolve the names of the pair into "Dinki" and "Nesh"
The four cameras are the twin Terminal Tracking Cameras (T2CAM), the Multicolor Visible Imaging Camera (MVIC), and the Long-Range Reconnaissance Imager (L’LORRI).
Puts into perspective the blurry mess if I try to photograph out of moving car window with a 70mm phone camI doubt you're seeing any of the orbit. Lucy was whizzing past. So its view changed as it went, but the two bodies were essentially in the same orientation as when they started. Without doing some back-of-the-envelope math, I would expect the period to be many hours.
I mean, they could be tidally locked. But I don't think we have any evidence one way or another.
Edit: As per the NASA page for this, the images in the moving GIF span a 70-second interval. So yeah, the rocks were essentially stationary over that time span.
Edit 2: The closest approach is given as 430 km with a relative velocity of 4.5 km/s which leads to a maximum slew rate of just over half a degree per second.
I think the answer here is...we don't know. This is the smallest we've directly imaged, so our data set is small. That question could lead to a future mission to try to find out, though I imagine that it would be tricky to plan enough encounters to answer it.I am a surgeon, not a physicist so apologies if this question is ridiculous but is it abnormal for something as small as a half mile wide asteroid to have enough mass / gravity to retain a satellite? Does this allow any assumptions to be made of what the asteroid is composed of? As in, if it’s that size and has a satellite the material has to have a certain density or higher?
Ballpark, the satellite is 3-5% of the mass of the primary. That's more than the moon, but not by a ton. And the only requirement that two objects remain bound is that their mutual attraction is more than perturbations from things like Jupiter. One did not necessarily capture the other. They may have been created at the same time either through a fracture of a larger parent and they've been traveling together ever since, or they both coalesced from the same ruble patch.Like others here, I’m also amazed a body 800m wide has enough gravity to have a satellite 200m wide. From the gif it looks like about 800m gap between them, hence 1.3km centre to centre.
If we model them as spherical rocky masses it should be quite simple to find the orbit times, the distances etc. My lunch hour ended 10 mins ago so I don’t have time to go through the calculations right now.
I am also not a physicist, but it isn't only gravitational force at work, but also material sciences and chance.I am a surgeon, not a physicist so apologies if this question is ridiculous but is it abnormal for something as small as a half mile wide asteroid to have enough mass / gravity to retain a satellite? Does this allow any assumptions to be made of what the asteroid is composed of? As in, if it’s that size and has a satellite the material has to have a certain density or higher?
I actually came back into this article to say the same thing (except the surgeon part). It's weird* to me that an Earthican foothill can trap a satellite in orbit.I am a surgeon, not a physicist so apologies if this question is ridiculous but is it abnormal for something as small as a half mile wide asteroid to have enough mass / gravity to retain a satellite? Does this allow any assumptions to be made of what the asteroid is composed of? As in, if it’s that size and has a satellite the material has to have a certain density or higher?
I think the more likely scenario is the one mentioned above - that the two objects originated from a single larger object.I actually came back into this article to say the same thing (except the surgeon part). It's weird* to me that an Earthican foothill can trap a satellite in orbit.
* Weird like unintuitive, not like I don't trust physics and this is all Big Asteroid's doing
In space, well away from anything, what action is there to pull two bodies apart? Using my ballpark numbers above, the gravitational force between these two is 40I actually came back into this article to say the same thing (except the surgeon part). It's weird* to me that an Earthican foothill can trap a satellite in orbit.
* Weird like unintuitive, not like I don't trust physics and this is all Big Asteroid's doing
Or a collision like formed the moon happened to the larger body. Some of the ruble escaped. Some coalesced back on the parent, and some formed the new satellite.I think the more likely scenario is the one mentioned above - that the two objects originated from a single larger object.
From what I read last night about this, they actually saw variations in the apparent brightness from Lucy's instruments leading up to the flyby. The suspected this meant that it was a binary, but were waiting for the flyby to confirm. Earlier telescope observations had seen variations in spectra (which they blamed on variation in surface composition as it rotated) and estimated the rate of rotation as 52.7 hours. The periodicity of the brightness variations Lucy observed were supposedly inline with this time scale.Ballpark, the satellite is 3-5% of the mass of the primary. That's more than the moon, but not by a ton. And the only requirement that two objects remain bound is that their mutual attraction is more than perturbations from things like Jupiter. One did not necessarily capture the other. They may have been created at the same time either through a fracture of a larger parent and they've been traveling together ever since, or they both coalesced from the same ruble patch.
And fine: spheres of 200m and 800m with a specific gravity of 3. That's 12e9 kg and 7.7e11 kg. At 1.3 km (assuming a circular orbit) you get a period of 34 hours. Or, as I guessed before, many hours.
If we're not seeing a good angle perpendicular to the two bodies, the distance could be longer. That would make the period longer.
The reason you think that is all the propaganda by Big Planet that doesn’t want you to believe the little ones are worthy of respect all on their own.I actually came back into this article to say the same thing (except the surgeon part). It's weird* to me that an Earthican foothill can trap a satellite in orbit.
* Weird like unintuitive, not like I don't trust physics and this is all Big Asteroid's doing
It's more like (1/4)^3 = 1/64 = 1.6%,Ballpark, the satellite is 3-5% of the mass of the primary. That's more than the moon, but not by a ton. And the only requirement that two
That would be for spheres of diameter ratios of 4. But since the number given were for the largest dimension, I was being conservative. But it's in the ballpark of the moon's ratio to earth's mass either way.It's more like (1/4)^3 = 1/64 = 1.6%,
For a hack estimate, I'll take my 34+ hour approximation as pretty close to the correct answer of 52.7 hours.From what I read last night about this, they actually saw variations in the apparent brightness from Lucy's instruments leading up to the flyby. The suspected this meant that it was a binary, but were waiting for the flyby to confirm. Earlier telescope observations had seen variations in spectra (which they blamed on variation in surface composition as it rotated) and estimated the rate of rotation as 52.7 hours. The periodicity of the brightness variations Lucy observed were supposedly inline with this time scale.