Skip to main content

NASA Selects Nine Potential Landing Sites for Artemis III Moon Mission.

 

This image displays nine candidate landing regions for NASA’s Artemis III mission, highlighting multiple potential sites for the first crewed Moon landing in over 50 years, with a background mosaic from the Lunar Reconnaissance Orbiter's Wide Angle Camera.


As NASA gears up for its first crewed Moon landing in over fifty years, the agency has unveiled an updated list of nine potential landing regions near the lunar South Pole for its upcoming Artemis III mission. These sites will undergo further scientific and engineering evaluations as part of the agency's preparations.


“Artemis will return humanity to the Moon and explore uncharted territories,” said Lakiesha Hawkins, assistant deputy associate administrator for the Moon to Mars Program Office. “Our selection of these regions underscores our commitment to ensuring crew safety while unlocking new scientific discoveries on the lunar surface.”


The refined candidate landing regions, selected by NASA’s Cross Agency Site Selection Analysis team in collaboration with science and industry partners, are as follows (in no particular order):


  • Peak near Cabeus B
  • Haworth
  • Malapert Massif
  • Mons Mouton Plateau
  • Mons Mouton
  • Nobile Rim 1
  • Nobile Rim 2
  • de Gerlache Rim 2
  • Slater Plain


These diverse geological sites offer a range of mission opportunities and could harbor permanently shadowed areas that may contain valuable resources, including water.


“The Moon’s South Pole presents an environment vastly different from that of the Apollo missions,” noted Sarah Noble, Artemis lunar science lead. “This region provides access to some of the Moon’s oldest terrain and areas that may contain water and other essential compounds, enabling groundbreaking scientific research.”


In selecting these regions, a multidisciplinary team analyzed extensive data from NASA’s Lunar Reconnaissance Orbiter alongside a wealth of lunar research. The selection criteria included scientific potential, terrain suitability, communication capabilities, and lighting conditions, ensuring optimal safety and accessibility for astronauts.


Jacob Bleacher, NASA’s chief exploration scientist, emphasized the significance of this mission: “Artemis III will mark the first time astronauts land in the Moon's south polar region, using a new lander and exploring a unique terrain. The goal is to find safe landing sites that also offer rich scientific opportunities.”


NASA's site assessment team plans to engage with the lunar science community through workshops and conferences to further refine their geological maps and assess the regional geology of the selected areas. The agency will continue to survey the lunar South Pole for both scientific value and mission potential, laying the groundwork for future Artemis missions, including Artemis IV and V, which will incorporate expanded scientific objectives and the Lunar Terrain Vehicle.


Ultimately, NASA aims to finalize landing sites for Artemis III in alignment with the mission's target launch dates, ensuring a successful and historic return to the Moon that includes landing the first woman, the first person of color, and international astronauts on the lunar surface, while paving the way for future human expeditions to Mars.

Comments

Popular posts from this blog

NASA/ESA Hubble Space Telescope Reveals New Details of the Orion Nebula’s Star Formation.

  This NASA/ESA Hubble Space Telescope image captures the Orion Nebula (Messier 42, M42), the nearest star-forming region to Earth, located about 1,500 light-years away. A captivating new image captured by the NASA/ESA Hubble Space Telescope offers an extraordinary look into the Orion Nebula, the nearest massive star-forming region to Earth. Located just 1,500 light-years away, this nebula is visible to the naked eye below the three stars forming Orion's "belt." The region is home to hundreds of newborn stars, including two protostars featured in the image: HOPS 150 and HOPS 153. Named after the Herschel Orion Protostar Survey, conducted with ESA’s Herschel Space Observatory, the protostars HOPS 150 and HOPS 153 provide key insights into the early stages of star formation. HOPS 150, visible in the upper-right corner of the image, is a binary star system, with two young stars orbiting one another. These protostars are surrounded by small dusty disks, where material from th...

New Method Detects Small Asteroids in Main Belt, Offering Insight for Planetary Defense.

  An international team of physicists, led by MIT researchers, has developed a groundbreaking method to detect small asteroids, as small as 10 meters in diameter, within the main asteroid belt. These space rocks, ranging from the size of a bus to several stadiums wide, were previously undetectable using traditional methods. The team's discovery, detailed in a paper published in Nature, could significantly improve tracking of potential asteroid impactors, aiding planetary defense efforts. The main asteroid belt, located between Mars and Jupiter, is home to millions of asteroids, but until now, scientists could only detect objects roughly a kilometer in diameter. The new detection technique, which utilizes the "shift and stack" method, is able to identify much smaller asteroids, even those far from Earth, enabling more precise orbital tracking. This breakthrough is crucial for planetary defense, allowing scientists to spot near-Earth objects that may pose a threat in the fu...

XSPECT Payload Successfully Validates Performance through Cas A Observation.

  The XSPECT instrument captures a detailed spectrum of the supernova remnant Cassiopeia A (Cas A), encompassing both the Galactic Cosmic Ray (GCR) background and the Cosmic X-ray Background (CXB). The flux observed above 8 keV predominantly results from the combined contributions of CXB and GCR. The presented spectrum, depicted in the figure, is derived from a cumulative integration time of 20 ksec, collected across multiple orbits, providing valuable insights into the X-ray emissions associated with Cas A. XPoSat, India's inaugural X-ray polarimetric mission, has achieved a significant as the XSPECT instrument captures its initial observations from the Cassiopeia A (Cas A) supernova remnant. Launched on January 1, 2024, XPoSat is equipped with two co-aligned instruments, namely the POLarimeter Instrument in X-rays (POLIX) and X-ray SPECtroscopy and Timing (XSPECT). This mission is designed to unravel the mysteries of cosmic X-ray sources. While POLIX focuses on examining X-ray po...