[astro-ph.EP] We present the results of a survey of previously uncharacterized near-Earth asteroids (NEAs) conducted between the second half of 2024 and the first months of 2026 using broadband BVRcIc […]
![Plot of the frequency vs. diameter for all asteroids with known or estimated rotation period with quality code 𝑈 ≥ 1. File data from the ALCDB of 1 Oct 2023, the last release (https://alcdef.org/). The two near-Earth asteroids, 2000 RD34 and 2000 DN8 (both with 𝑈 = 1), are shown together with the five LSFR from Rubin observations (red) and the candidate LSFR or almost candidate (due to borderline diameter as for 2015 RG36 and 2024 WB), which we have characterized at the Loiano Astronomical Station, managed by INAF-OAS in Italy (cyan). The curves for the rubble pile model with cohesion strength are from Eq. 12 (Sánchez and Scheeres, 2014). Our candidates LSFR has a cohesive strength between 102–104 Pa. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Photometric.png?resize=1200%2C721&ssl=1)
[astro-ph.EP] We present the results of a survey of previously uncharacterized near-Earth asteroids (NEAs) conducted between the second half of 2024 and the first months of 2026 using broadband BVRcIc […]