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The spacecraft's laser range finder, or LRF, experienced an anomaly that prevented Resilience from obtaining valid ...
NASA's Lunar Reconnaissance Orbiter (LRO) has imaged the crash site of Resilience, a moon lander built and operated by the Tokyo-based company ispace. Resilience tried to touch down on June 5 in the ...
The Japanese company's Resilience spacecraft aimed to make a soft touchdown in the Mare Frigoris ("Sea of Cold") region of the moon's near side today (June 5) at 3:17 p.m. EDT (1917 GMT; 4:17 a.m ...
This image provided by NASA shows an annotation indicating the impact site for ispace's Resilience lunar lander, seen by the Lunar Reconnaissance Orbiter Camera on June 11, 2025. — Photo from ...
A NASA spacecraft around the moon has photographed the crash site of a Japanese company’s lunar lander. NASA released the pictures Friday, two weeks after ispace’s ...
The moon is pictured half-lit during its first quarter phase. The locations of the Aristotles and Eudoxus craters are shown close to Mare Frigoris towards the north, while the Sea of Tranquility ...
Mare Frigoris is significantly flatter than the Atlas crater region, potentially offering easier-to-navigate terrain. Ispace said in a statement that the new landing site was chosen because it ...
Resilience, which is 7.5 feet (2.3 meters) tall and 8.5 feet (2.6 m) wide, is targeting Mare Frigoris, a vast, relatively smooth basaltic plain in the moon's northern hemisphere.
Mare Frigoris is significantly flatter than the Atlas crater region, potentially offering easier-to-navigate terrain. Ispace said in a statement that the new landing site was chosen because it ...
The Mare Frigoris, also known as the Cold Sea, is a region near the Moon’s north pole which scientists have been studying in depth. They completed a survey of more than 12,000 images showing the ...
The study area, which is an elongated mare, Mare Frigoris and northern Mare Imbrium, was mapped and characterized into 27 units based on multi-source data, including spectrum, terrain, and element ...
The most prominent candidate ring structures are the mare shorelines and scarps on the western edge of Oceanus Procellarum and the northern edge of Mare Frigoris 5 (Fig. 1a; Extended Data Fig. 1).