The Lunar Orbiter Laser Altimeter (LOLA) provides a precise global lunar topographic model and geodetic grid that serves as the foundation of essential lunar understanding. This aids future missions by providing topographical data for safe landings and enhance exploration-driven mobility on the Moon. LOLA also contributes to decisions as to where to explore by looking at the evolution of the surface.
LOLA fully achieves three LRO measurement objectives and addresses two other. LOLA will provide all the data necessary to select intriguing, safe landing sites, while providing the reference system needed to navigate to those sites.
LOLA builds on extensive spaceflight heritage, including the Mercury Laser Altimeter (MLA) and the Mars Orbiter Laser Altimeter (MOLA). The LOLA measurement team has 15 years of altimetry experience that includes providing MOLA data to the Mars Exploration Rover site-selection teams.
LOLA works by propagating a single laser pulse through a Diffractive Optical Element (DOE) that splits it into five beams.
These beams then strike and are backscattered from the lunar surface. For each beam, LOLA measures time of flight (range), pulse spreading (surface roughness), and transmit/return energy (surface reflectance). With its two-dimensional spot pattern, LOLA unambiguously determines slopes along-track and across-track.Image Above : LOLA Projection surface
In a 50km polar orbit, pulsing the laser at 28 Hz creates an ~50m-wide swatch of five topographic profiles. Swaths will have 1.25km separation at the equator, with [complete polar coverage beyond +/-86 degrees latitude.] Raw measurements are transmitted to Earth for analysis.
LOLA's robust link margin provides ample reserve to accommodate uncertainties in lunar surface roughness and albedo, while providing operational flexibility to the LRO mission.