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thunkii.bsky.social

@thunkii.bsky.social
16 followers 9 following 17 posts
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thunkii.bsky.social @thunkii.bsky.social · 21/08/2026
I got Pure Land once in an untracked attempt.
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thunkii.bsky.social @thunkii.bsky.social · 20/08/2026
Tried this with 100 attempts, and obtained the following distribution:
The one true religion, as suggested by Google Gemini with the wording by hikikomorphism. Pie charts show number of suggestions out of 100 attempts.
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Reposted by @thunkii.bsky.social
astrafoxen @astrafoxen.bsky.social · 15/06/2026
Last year I rewrote Wikipedia's article on Makemake and it's now featured on the front page!! i spent 2 months hyperfixating on this topic and doing all the research and writing. It was SO worth it :D Special thanks to @renerpho.bsky.social & others for reviewing it ^^ (1/12 thread) 🔭 #planetsci
A screenshot of the "Today's featured article" section on the Main Page of Wikipedia. The section, highlighted in green, features an excerpt from the Wikipedia article on Makemake:

"Makemake is a dwarf planet orbiting the Sun beyond Neptune. It has a diameter 60% that of Pluto, and is the fourth-largest trans-Neptunian object and the largest member of the Solar System's classical Kuiper belt, a disk of icy bodies beyond Neptune's orbit. Its discovery on March 31, 2005, by American astronomers Mike Brown, Chad Trujillo and David Rabinowitz at Palomar Observatory contributed to the reclassification of Pluto as a dwarf planet in 2006. Makemake's surface, like Pluto's, is largely covered by frozen methane and stained reddish-brown by tholins. It has one known satellite, unnamed, whose orbit suggests that Makemake's rotation has a high axial tilt. Makemake shows evidence of geochemical activity and cryovolcanism, which has led scientists to suspect that it might harbor a subsurface ocean of liquid water. No high-resolution images of its surface exist because it has not been visited up close by a space probe."

https://en.wikipedia.org/wiki/Makemake
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thunkii.bsky.social @thunkii.bsky.social · 24/05/2026
A thread of explanatory notes is in my thread from then: bsky.app/profile/thun...
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thunkii.bsky.social @thunkii.bsky.social · 24/05/2026
After some minor fixes I made to the visualization of 1,509,413 asteroids, and their position in space as of last week, it's good to go for Wikipedia! commons.wikimedia.org/wiki/File:As...
Plot of the position in space, as of the instant of midnight ephemeris time 15 May 2026, of 1,509,325 asteroids. The size of each circle represents the square root of the asteroid's diameter, and is not to scale with their orbital distance. Types of asteroids are color-coded; white are main-belt asteroids, pink are Trojan asteroids ('Greeks' at L4 and 'Trojans' at L5 lagrange points), purple are Hilda asteroids, orange and yellow are Mars-crossing and near-Earth asteroids, and green dots are comets. The inner planets and Jupiter are labeled in gold. The top chart represents a view top-down into the plane of the solar system, and the bottom chart is a side view.
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thunkii.bsky.social @thunkii.bsky.social · 15/05/2026
As before, here is a full res version: commons.wikimedia.org/wiki/File:As...
commons.wikimedia.org
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thunkii.bsky.social @thunkii.bsky.social · 15/05/2026
Positions, sizes, and magnitudes of asteroids are derived from the JPL Small Bodies Database, with orbital elements integrated from the provided epoch (mostly November 2025). Planet positions are from DE440; coordinates are in the J2000 ecliptic, with the +x axis pointing to the vernal equinox.
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thunkii.bsky.social @thunkii.bsky.social · 15/05/2026
We can also see that the plane of the main belt is tilted slightly away from Earth's orbit and closer to the Solar System's invariable plane. The same is true of the classical Kuiper belt. The biggest yellow dot between Earth and Mars's orbit is 433 Eros, visited by NEAR Shoemaker in 2001.
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thunkii.bsky.social @thunkii.bsky.social · 15/05/2026
The side view of the asteroid belt (bottom) shows that it's more of a donut, though it is far emptier--space is big, and most asteroids are found several million km from each other. The pink Trojans can have high-inclination orbits, due to the stability of Jupiter's L4 and L5 Lagrange points.
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thunkii.bsky.social @thunkii.bsky.social · 15/05/2026
Other categories of asteroids are harder to spot. The 'Hildas triangle' in purple results from a 3:2 orbital resonance keeping them away from Jupiter. Near-Earth asteroids in red and yellow tend to be much smaller but can pose a threat to Earth, as do various short-period comets (green).
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thunkii.bsky.social @thunkii.bsky.social · 15/05/2026
There are more ways to visualize asteroids, such as their location in space today. Here are 1,509,413 of them, plotted to scale with each other (but not to the planets or their orbits). We can clearly see the main belt in white and Trojan asteroids in pink.
A view from above the plane of the solar system (top) or in its plane (bottom) onto the asteroid belt, showing 1.5 million asteroids to scale with each other, with their positions as of 15 May 2026 (but greatly enlarged compared to their orbits). The inner planets and Sun is shown in gold, while the main belt is visible as a donut-shaped cloud in white, and Trojan asteroids are in pink clouds 60 deg ahead or behind Jupiter. Other categories of asteroids are seen on closer inspection, including the Hildas triangle (purple), outer-belt/Cybele asteroids (light blue), Hungarias (orange), Amors and Mars-crossers (yellow), and near-Earth asteroids (red), as well as scattered comets (green).
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Reposted by @thunkii.bsky.social
Luke Bones 🦴🦴 @lukemeister.bsky.social · 14/05/2026
🧵 Link to high-resolution versions of inclination and eccentricity vs. semi-major axis at end of thread Proper elements from David Nesvorný's catalog www2.boulder.swri.edu/~davidn/Prop... David's paper: iopscience.iop.org/article/10.3...
iopscience.iop.org
A Census before Rubin of Asteroid Families in the Main Belt
A Census before Rubin of Asteroid Families in the Main Belt, Nesvorný, David
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thunkii.bsky.social @thunkii.bsky.social · 14/05/2026
These images got ate by compression. Full-size versions are on Commons: commons.wikimedia.org/wiki/File:As... commons.wikimedia.org/wiki/File:As...
commons.wikimedia.org
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thunkii.bsky.social @thunkii.bsky.social · 14/05/2026
Asteroid proper elements are from Nesvorný et al. 2025, www2.boulder.swri.edu/~davidn/Prop.... Diameters are derived from the JPL Small Bodies Database (SBDB) where available, or otherwise guessed from the absolute magnitude and mean albedo of each sub-belt.
www2.boulder.swri.edu
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thunkii.bsky.social @thunkii.bsky.social · 14/05/2026
Asteroids range in size from the four largest: Vesta (inner belt), Ceres and Pallas (mid belt), and Hygiea (outer belt), to millions of kilometer-size rocks that are barely one pixel across. If you look closely at top left of the inclination plot, you can see the small but bright Hungarias (orange).
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thunkii.bsky.social @thunkii.bsky.social · 14/05/2026
Here's another graph, showing the eccentricity vs the semi-major axis. While most asteroids are ejected from the major resonances with Jupiter, forming the Kirkwood gaps, some are trapped there and gradually excited onto planet-crossing orbits.
A plot of eccentricity vs semi-major axis (in AU) and orbital period (in years) of 1,249,051 asteroids in the asteroid belt. The sizes of each circle correspond to the asteroid's diameter. The main belt is shown in various shades of white, with Hungaria asteroids in orange and Cybele asteroids in blue. Orbital resonances with Jupiter are marked in red, and most of these resonances either show no asteroids or a vertical line of 'trapped' asteroids.
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thunkii.bsky.social @thunkii.bsky.social · 14/05/2026
This is a graph of the inclination vs semi-major axis (distance from the sun) of 1,249,051 asteroids in the asteroid belt. Using proper elements allows us to see the belt's fine structure, including asteroid families that are fragments of past collisions. Each asteroid is (roughly) to scale.
A plot of 1,249,051 asteroids within the asteroid belt, showing (proper) inclination vs semi-major axis (in AU) and orbital period (in years). The size of the circles is proportional to the diameter of each asteroid. The main asteroid belt is shown in shades of white, while Hungaria asteroids are in orange and the Cybele asteroids are in blue. Red markers note the position of the 1:4, 1:3, 3:8, 2:5, 3:7, 4:9, 5:11, 1:2, and 3:5 orbital resonances with Jupiter.
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thunkii.bsky.social @thunkii.bsky.social · 03/04/2026
actually closer to 414 m/s; this will occur at approximately 23:30 TDB on 6 April
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thunkii.bsky.social @thunkii.bsky.social · 03/04/2026
according to JPL Horizons, minimum speed in the Earth-centered inertial frame is about 416 m/s when it's swinging around the back side of the Moon. Basically the flyby speed cancels out the Moon's orbital speed.
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