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#2024yr4

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Probability of #Asteroid #2024YR4 hitting the #Moon increases
Scientists improve knowledge by 20% thanks to #JamesWebb #Space #Telescope data
#NASA said data from the #JWST "improved our knowledge of where the asteroid will be on Dec. 22, 2032, by nearly 20 percent." The upshot is that there is now a 4.3% possibility that the asteroid will hit the Moon in 7.5 years' time, although it wouldn't alter the natural satellite's orbit.
theregister.com/2025/06/10/ast

The Register · Probability of Asteroid 2024 YR4 hitting the Moon increasesBy Richard Speed

To reiterate a point about asteroid impact probabilities:

Different data weights and subsets will produce significantly different estimates, even though they all will converge to either 0 or 100% impact probability eventually.

For #2024YR4 and the Moon, we will just have to be patient until 2028.

Keine Gefahr für die Erde, aber vielleicht für den Mond..?🌔Der #asteroid #2024YR4 bleibt im Blick der Planetary Defense Community.🔭Klingt nach einem epischen Namen?Nicht nur der ist episch, auch die Aufgaben sind es.Mehr darüber gibt es im aktuellen Beitrag von Josis Blick in den Himmel👉sternwarte-goennsdorf.de/josi/ .Das Foto des James-Webb-Teleskops zeigt den Asteroiden.Unspektakulär?Der Brocken ist so groß wie ein Gebäude mit 15 Stockwerken!😮
Fotocredits: #nasa #esa #csa STScI, A. Rivkin (JHU APL)

Continued thread

Davide Farnocchia reviews #2024YR4:

63 observatories, >500 observations.

3.8% chance of lunar impact in 2032 December, with the last observations for this year still pending.

It will likely require waiting until 2028 to resolve the lunar impact possibility. But it cannot impact Earth.

NASA doubles odds of Moon hitting Near-Earth Asteroid [2024 YR4].

"Experts at NASA’s Center for Near Earth Object Studies at the agency’s Jet Propulsion Laboratory have updated [2024 YR4]’s chance of impacting the Moon on December 22, 2032 from 1.7 to 3.8 percent," the agency said.

science.nasa.gov/blogs/planeta

Aardscheerder 2024 YR4 is vermoedelijk afkomstig uit de hoofdgordel

Astronomen hebben met behulp van het GMOS-instrument (Gemini Multi-Object Spectrograph) aan de Gemini Zuid-telescoop bepaald dat de recent gevonden aardscheerder 2024 YR4 een van de grootste objecten in de recente geschiedenis is dat op de Maan kan ins

kuuke.nl/aardscheerder-2024-yr

Continued thread

Here are three orthogonal views of a convex shape model of asteroid 2024 YR4 from the paper - a top down view (X-Y) and 2 side views (X-Z and Y-Z).

The asteroid is spinning around the Z axis.

So, what are the physical processes responsible for this flattish shape? Was the asteroid more spherical in the distant past?

Paper: arxiv.org/html/2503.05694v2
#2024YR4
5/n

I read people being surprised that #2024YR4 is shaped like an irregular block.

Such a shape is typical for small rapidly-spinning asteroids, which are held together by tensile strength rather than by gravity.

For a similarly-sized comparison, consider 2015 HM10: public.nrao.edu/news/radar-201

National Radio Astronomy ObservatoryImage Release: Radar Observations Shine New Light on Near-Earth Asteroid - National Radio Astronomy ObservatorySummer school astronomers image near-Earth asteroid.

The discovery and characterization of Earth-crossing asteroid #2024YR4: arxiv.org/abs/2503.05694 -> Astronomers Trace Earth-Crossing Asteroid to Surprising Origin: keckobservatory.org/2024-yr4/ (namely that it's a solid, stony type that likely originated from an asteroid family in the central Main Belt between Mars and Jupiter, a region not previously known to produce Earth-crossing asteroids).

arXiv.orgThe discovery and characterization of Earth-crossing asteroid 2024 YR$_4$We describe observations and physical characteristics of Earth-crossing asteroid 2024 YR$_4$, discovered on 2024 December 27 by the Asteroid Terrestrial-impact Last Alert System. The asteroid has semi-major axis, $a$ = 2.52 au, eccentricity, $e$ = 0.66, inclination $i$ = 3.41$^{\circ}$, and a $\sim$0.003 au Earth minimum orbit intersection distance. We obtained g, r, i, and Z imaging with the Gemini South/Gemini Multi-Object Spectrograph on 2025 February 7 and Y and J imaging with the Keck/Multi-Object Spectrometer For Infra-Red Exploration on 2025 February 12. We measured a g-i spectral slope of 13$\pm$3 $\%$/100 nm, and color indices g-r = 0.70 $\pm$ 0.10, r-i = 0.25$\pm$0.06, i-Z = -0.27 $\pm$ 0.10, and Y-J = 0.41 $\pm$ 0.10. 2024 YR$_4$ has a spectrum that best matches R-type and Sa-type asteroids and a diameter of $\sim$30-65 m using our measured absolute magnitude of 23.9 $\pm$ 0.3 mag, and assuming an albedo of 0.15-0.4. The lightcurve of 2024 YR$_4$ shows $\sim$0.4 mag variations with a rotation period of $\sim$1170 s. We use photometry of 2024 YR$_4$ from Gemini and other sources taken between 2024 December to 2025 February to determine the asteroid's spin vector and shape, finding that it has an oblate, $\sim$3:1 a:c axial ratio and a pole direction of $λ$, $β$ = $\sim$42$^{\circ}$, $\sim$-25$^{\circ}$. Finally, we compare the orbital elements of 2024 YR$_4$ with the NEO population model and find that its most likely sources are resonances between the inner and central Main Belt.