Lunar Reconnaissance Orbiter (LRO): Observations for Lunar Exploration and Science

By R. Vondrak, J. Keller, G. Chin, J. Garvin. 2010

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Orbit determination of the Lunar Reconnaissance Orbiter (2012, methodology): “This is technically a measure of precision and not of the orbit accuracy itself (as required for the LRO position knowledge; Vondrak et al. 2010).”
Gravity and Topography of the Terrestrial Planets (2015, background): “Thus, although regional topographic models have been constructed for some moons and asteroids (such as Phobos (Wählisch et al., 2010), 433 Eros (Gaskell et al., 2008; Zuber et al., 2000a), Itokawa (Abe et al., 2006; Gaskell et al., 2008), Vesta ( Jaumann et al., 2012), Ganymede (Giese et al.,…”
Lunar equatorial surface temperatures and regolith properties from the Diviner Lunar Radiometer Experiment (2012, unknown): “The collection of such data has been a primary goal of the Lunar Reconnaissance Orbiter (LRO) mission [Vondrak et al., 2010].”
The global surface temperatures of the Moon as measured by the Diviner Lunar Radiometer Experiment (2017, unknown): “…). n V t r w t s a o ( b e o a c t l r r o s t r i l v n m a g c t h s 2 2 a ( i p t c b t t m n m 2 t o ∼ o c ∼ i ∼ E n w D ( 2 i d s p t a s 1 d o e s t i i p s t R G L 6 c E o l aissance Orbiter (LRO) ( Chin et al., 2007; Tooley et al., 2010; ondrak et al., 2010 ).”