Talk:469219 Kamoʻoalewa

Talk:469219 Kamoʻoalewa

Appearance and shape: Reply

← Previous revision Revision as of 19:15, 27 April 2026
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Presumably we have no way to tell how much of the lightcurve variation is due to non-spherical shape vs variations in surface albedo. Could any current telescope (or radar) 'see' even the orientation of its axis of rotation ? - [[User:Rod57|Rod57]] ([[User talk:Rod57|talk]]) 10:52, 23 December 2017 (UTC)
Presumably we have no way to tell how much of the lightcurve variation is due to non-spherical shape vs variations in surface albedo. Could any current telescope (or radar) 'see' even the orientation of its axis of rotation ? - [[User:Rod57|Rod57]] ([[User talk:Rod57|talk]]) 10:52, 23 December 2017 (UTC)
: Have any sources published lightcurve plots (maybe with error bars) - [[User:Rod57|Rod57]] ([[User talk:Rod57|talk]]) 11:07, 23 December 2017 (UTC)
: Have any sources published lightcurve plots (maybe with error bars) - [[User:Rod57|Rod57]] ([[User talk:Rod57|talk]]) 11:07, 23 December 2017 (UTC)
:i think this might be what you're looking for?
:https://www.aanda.org/articles/aa/full_html/2024/12/aa51407-24/F2.html [[User:MrAstronomy101|MrAstronomy101]] ([[User talk:MrAstronomy101|talk]]) 19:15, 27 April 2026 (UTC)


== Pronunciation ==
== Pronunciation ==