Photometry and polarimetry of Jupiter at large phase angles

Icarus ◽  
1984 ◽  
Vol 58 (1) ◽  
pp. 35-73 ◽  
Author(s):  
Peter H. Smith ◽  
Martin G. Tomasko
Keyword(s):  
2018 ◽  
Vol 611 ◽  
pp. A31 ◽  
Author(s):  
Daisuke Kuroda ◽  
Masateru Ishiguro ◽  
Makoto Watanabe ◽  
Sunao Hasegawa ◽  
Tomohiko Sekiguchi ◽  
...  

We present a unique and significant polarimetric result regarding the near-Earth asteroid (152679) 1998 KU2, which has a very low geometric albedo. From our observations, we find that the linear polarization degrees of 1998 KU2are 44.6 ± 0.5% in theRCband and 44.0 ± 0.6% in theVband at a solar phase angle of 81.0°. These values are the highest of any known airless body in the solar system (i.e., high-polarization comets, asteroids, and planetary satellites) at similar phase angles. This polarimetric observation is not only the first for primitive asteroids at large phase angles, but also for low-albedo (<0.1) airless bodies. Based on spectroscopic similarities and polarimetric measurements of materials that have been sorted by size in previous studies, we conjecture that 1998 KU2has a highly microporous regolith structure comprising nano-sized carbon grains on the surface.


Icarus ◽  
1978 ◽  
Vol 33 (3) ◽  
pp. 558-592 ◽  
Author(s):  
M.G. Tomasko ◽  
R.A. West ◽  
N.D. Castillo
Keyword(s):  

1991 ◽  
Vol 11 (9) ◽  
pp. 111-115 ◽  
Author(s):  
Peter Richter ◽  
Manfred Scholer
Keyword(s):  

2018 ◽  
Vol 620 ◽  
pp. A179 ◽  
Author(s):  
Maxim Zheltobryukhov ◽  
Ekaterina Chornaya ◽  
Anton Kochergin ◽  
Gennady Kornienko ◽  
Alexey Matkin ◽  
...  

Context. The near-Earth asteroid (3200) Phaethon occasionally reveals a comet-like activity. It is a parent body to the Geminid meteor shower and considered as a target for the space mission called Demonstration and Experiment of Space Technology for Interplanetary Voyage Phaethon Flyby Dust Science, DESTINY+. Aims. We aim to characterize Phaethon through measurements of the degree of linear polarization P measured on Phaethon at large phase angles on its closest approach to Earth on December 17, 2017. These observations allow a more accurate estimation of the maximum value of the degree of linear polarization Pmax of Phaethon, and therefore, of studying the Umov effect. Methods. We performed polarimetric measurements of Phaethon at large phase angles α and thus constrained its Pmax. We also estimated the geometric albedo a based on the data available in the literature. The obtained Pmax and A were analysed with the Umov effect previously derived for the Moon that establishes an inverse linear correlation between log(Pmax) and log(A) in the lunar regolith. Results. Our polarimetric observations of Phaethon in the visible reveal the degree of linear polarization P ≈ (17.23 ± 2.00)% at α ≈ 57.9° and P ≈ (31.86 ± 2.00)% at α ≈ 73.2°, which demonstrates no significant wavelength dependence within the error bars of our measurements (± 2%). These data, when combined with what has previously been reported in the literature, suggests at least three types of polarimetric response on Phaethon. For two of them, we infer the maximum linear polarization to be Pmax ≈ 57.9%, occurring at αmax = 131° and Pmax ≈ 44.5% occurring at αmax = 127°. We estimate the geometric albedo (adjusted to α = 3°) to be AR = 0.075 ± 0.007 in the R filter, which appears to be consistent with dark F-type asteroids, as which Phaethon was first classified. We examine the Umov diagrams previously inferred for lunar regolith and find that they are hardly applicable to Phaethon and therefore not to other asteroids either.


1980 ◽  
Vol 85 (A11) ◽  
pp. 5891 ◽  
Author(s):  
M. G. Tomasko ◽  
R. S. McMillan ◽  
L. R. Doose ◽  
N. D. Castillo ◽  
J. P. Dilley
Keyword(s):  

Icarus ◽  
2017 ◽  
Vol 296 ◽  
pp. 117-122 ◽  
Author(s):  
Yuriy Shkuratov ◽  
Evgenij Zubko ◽  
Gorden Videen
Keyword(s):  

Author(s):  
M. G. Tomasko ◽  
R. S. McMillan ◽  
L. R. Doose ◽  
N. D. Castillo ◽  
J. P. Dilley
Keyword(s):  

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