1. RISE Project,National Astronomical Observatory 2. Faculty of Engineering,Iwate University, 3. Department of Astronomical Science,The Graduate University for Advanced Studies(SOKENDAI) 4. Wireless Network Research Institute,National Institute of Information and Communications Technology 5. Department of Earthand Space Science,Osaka University
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Received
Published Online
2022-05-20
2022-05-20
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Abstract
We investigated basic characteristics of the telescope for In-situ Lunar Orientation Measurement (ILOM), such as the centroid accuracy and the effects of temperature change, tilt and ground vibrations, by laboratory experiments using a Bread Board Model and by simulations. We have a prospect to observe the lunar rotation on the lunar surface with the accuracy of 1 milliarcsecond. We will make test observations on the ground in order to evaluate overall characteristics with the target accuracy of better than 0.1 arcseconds.