TY - JOUR

T1 - Physical properties of near-Earth asteroid (2102) Tantalus from multiwavelength observations

AU - Rozek, Agata

AU - Lowry, Stephen C.

AU - Rozitis, Benjamin

AU - Dover, Lord R.

AU - Taylor, Patrick A.

AU - Virkki, Anne

AU - Green, Simon F.

AU - Snodgrass, Colin

AU - Fitzsimmons, Alan

AU - Campbell-White, Justyn

AU - Sajadian, Sedighe

AU - Bozza, Valerio

AU - Burgdorf, Martin J.

AU - Dominik, Martin

AU - Jaimes, R. Figuera

AU - Hinse, Tobias C.

AU - Hundertmark, Markus

AU - Jorgensen, Uffe G.

AU - Longa-Pena, Penelope

AU - Rabus, Markus

AU - Rahvar, Sohrab

AU - Skottfelt, Jesper

AU - Southworth, John

PY - 2022/8/11

Y1 - 2022/8/11

N2 - Between 2010 and 2017, we have collected new optical and radar observations of the potentially hazardous asteroid (2102) Tantalus from the ESO NTT and Danish telescopes at the La Silla Observatory, and from the Arecibo planetary radar. The object appears to be nearly spherical, showing a low-amplitude light-curve variation and limited large-scale features in the radar images. The spin-state is difficult to constrain with the available data; including a certain light-curve subset significantly changes the spin-state estimates, and the uncertainties on period determination are significant. Constraining any change in rotation rate was not possible, despite decades of observations. The convex light curve-inversion model, with rotational pole at lambda = 210 degrees +/- 41 degrees and beta = -30 degrees +/- 35 degrees, is more flattened than the two models reconstructed by including radar observations: with prograde (lambda= 36 degrees +/- 23 degrees, beta = 30 degrees +/- 15 degrees), and with retrograde rotation mode (lambda = 180 degrees +/- 24 degrees, beta = -30 +/- 16 degrees). Using data from WISE, we were able to determine that the prograde model produces the best agreement in size determination between radar and thermophysical modelling. Radar measurements indicate possible variation in surface properties, suggesting one side might have lower radar albedo and be rougher at the centimetre-to-decimetre scale than the other. However, further observations are needed to confirm this. Thermophysical analysis indicates a surface covered in fine-grained regolith, consistent with radar albedo, and polarisation ratio measurements. Finally, geophysical investigation of the spin-stability of Tantalus shows that it could be exceeding its critical spin-rate via cohesive forces.

AB - Between 2010 and 2017, we have collected new optical and radar observations of the potentially hazardous asteroid (2102) Tantalus from the ESO NTT and Danish telescopes at the La Silla Observatory, and from the Arecibo planetary radar. The object appears to be nearly spherical, showing a low-amplitude light-curve variation and limited large-scale features in the radar images. The spin-state is difficult to constrain with the available data; including a certain light-curve subset significantly changes the spin-state estimates, and the uncertainties on period determination are significant. Constraining any change in rotation rate was not possible, despite decades of observations. The convex light curve-inversion model, with rotational pole at lambda = 210 degrees +/- 41 degrees and beta = -30 degrees +/- 35 degrees, is more flattened than the two models reconstructed by including radar observations: with prograde (lambda= 36 degrees +/- 23 degrees, beta = 30 degrees +/- 15 degrees), and with retrograde rotation mode (lambda = 180 degrees +/- 24 degrees, beta = -30 +/- 16 degrees). Using data from WISE, we were able to determine that the prograde model produces the best agreement in size determination between radar and thermophysical modelling. Radar measurements indicate possible variation in surface properties, suggesting one side might have lower radar albedo and be rougher at the centimetre-to-decimetre scale than the other. However, further observations are needed to confirm this. Thermophysical analysis indicates a surface covered in fine-grained regolith, consistent with radar albedo, and polarisation ratio measurements. Finally, geophysical investigation of the spin-stability of Tantalus shows that it could be exceeding its critical spin-rate via cohesive forces.

KW - techniques: photometric

KW - techniques: radar astronomy

KW - minor planets, asteroids: individual: (2102) Tantalus

KW - methods: observational

KW - RADAR SURVEY

KW - PLANETARY SURFACES

KW - SPIN-UP

KW - YORP

KW - YARKOVSKY

KW - OBJECTS

KW - MODEL

KW - STATE

KW - ACCELERATION

KW - ROTATION

U2 - 10.1093/mnras/stac1835

DO - 10.1093/mnras/stac1835

M3 - Journal article

VL - 515

SP - 4551

EP - 4564

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 3

ER -