May 14, 2026
Moon's Ice Mysteries, Aussie Rover's Lunar Mission, and a Distant World's Unexpected Atmosphere
SpaceTime Series 29 Episode 58 *Unlocking the mystery of water on the Moon New evidence suggests that water ice has been accumulating on the Moon for at least one and a half billion years. *An Australian Lunar rover to land on the Moon in 2030 NASA has scheduled the Australian developed ROOVER lunar rover to fly to the Moon in 2030 as part of the Intuitive Machines CT-4 mission to the lunar South Pole. *Discovery of an atmosphere on a distant frozen world that shouldn’t have one Astronomers have discovered a thin atmosphere on a distant world far beyond Neptune where no atmosphere should exist. *The Science Report Claims micro and nano-plastics in the atmosphere may contribute to global warming. Evidence of copper mining going back over 5000 years. Study shows astronauts need extra time to remember how to hold things when they get back to Earth. Skeptics guide to the limits of anecdotal evidence rather than rigorous scientific testing. Our Guests This Week: Associate Professor Ben Montet from the University of New South Wales Bepi Columbo mission MIXS principle investigator Emma Bunce University of Leicester Bepi Columbo mission SIMBIO-SYS principle investigator Gabriele Cremonese Bepi Columbo mission MPO-MAG investigator Daniel Heyner Technical University of Braunschweig And our regular guests: Alex Zaharov-Reutt from techadvice.life Tim Mendham from Australian Skeptics 🌏 Get Our Exclusive NordVPN deal here ➼ www.bitesz.com/nordvpn . The discounts and bonuses are incredible! And it’s risk-free with Nord’s 30-day money-back guarantee! ✌ If you’d like to support the podcast and gain access to bonus content by becoming a SpaceTime crew member, you can do just that through premium versions on Patreon, Spotify and Apple Podcasts. Details on the Support page on our website https://www.bitesz.com/show/spacetime/support/
The Astronomy, Space, Technology & Science News Podcast.
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This is Spacetime Series twenty nine, episode fifty eight, well
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broadcast on the fifteenth of May twenty twenty six. Coming
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up on Space Time, unlocking the mystery of water on
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the Moon, a new Australian built lunarova to land on
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the Moon in twenty thirty, and discovery of an atmosphere
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on a distant frozen world which shouldn't have one. All
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that and more coming up on Spacetime.
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Welcome to space Time with Stewart Gary.
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New evidence suggests that ice has been accumulating on the
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Moon for at least one and a half billion years.
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The findings reported in the General Nature Astronomy are also
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put into the best places on the learner's surface to
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find it. More than half a century after Apollo seventeen
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made the last manned lunar landing, a new space race
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to the Moon is underway. Last month successful Artemis two
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mission by the United States, and with both the United
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States and China now aiming to establish their own permanent
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bases there. Unlikely Apollo program, during which American astronauts landed
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at six different sites on the lunar surface, twenty first
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century emissions are all focused on a single location the
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Moon's south pole. Spaceflight pioneer Robert Goddard proposed over a
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century ago that water ice deposits might exist at the
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lunar poles, and indirect evidence collected over the past twenty
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years has lent support to this hypothesis. In space exploration,
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water ice is a highly sought after resource. It can
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be processed into liquid water for drinking and irrigation, split
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into hydrogen oxygen for us as rocket fuel, and even
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used to study the history of celestial bodies in our
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Solar system. Now, researchers have uncovered new evidence showing that
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ice has been gradually accumulating at the Moon's poles for
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at least nest one and a half billion years in
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ancient cold traps on the lunar surface. Unlike Earth, whose
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tilted axis causes the Sun's position in the sky to
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change throughout the year, the Moon has almost no tilt,
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and so the Sun's always positioned approximately above the lunar equator. Now,
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if you're standing at one of the lunar poles, you'd
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see the Sun staying close to the horizon as it
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completes a monthly cycle, rather than rising and setting as
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it does here on Earth. As a result, sunlight can't
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reach and warm the deep permanently shadowed floors of craters
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at the lunar poles. But this wasn't always the case.
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In the distant past, the Moon did have a much
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greater axial tilt, but over the last few billion years
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it's been straightening out. In twenty twenty three, scientists showed
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that as the Moon's tilt decreased, more and more craters
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near the poles became permanently shadowed and cooled dramatically. By
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calculating when each crater lost its exposure to sunlight, the
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authors were able to deduce the age of each permpanly
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shadowed region. They set out to examine whether there was
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a connection between the age of a permanently shadowed region
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and the proportion of its area covered by ice. Ice
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reflects more ultraviolet light at certain wavelengths than the Moon's
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normal rocky surface, and that makes it possible to infer
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where it's located. And ultraviolet light provides an advantage because
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it emanates not only from the Sun but also from
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distant stars, and so it can enter permanently shattered areas.
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The author's analyzed data collected by NASA's Lunar Reconnaissance Orbital
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which is equipped with the laser optimeter and alignment Alpha
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mapping instrument, which is sensitive to ultraviolet radiation. The spacecraft's
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been orbiting and mapping the Moon since two thousand and nine,
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and the new data is confirmed that permanently shadowed craters
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near the Moon's south pole are promising locations to find
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water ice. The authors found that while these coal traps
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have been accumulating water ice for at least the last
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one and a half billion years, not all are equally effective.
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For example, the well known Shackleton Crater, which is very
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close to the Luna south pole, has been too warm
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for much of lunar Hitty Street to collect ice. However,
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Harworth Crater has acted as an efficient ice trap for
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billions of years and has therefore been identified as a
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prime target for future landed missions. One of the studies
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authors of Deed Aronson from Israel's Weisman Institute, says the
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data shows that the earlier origion became shadowed, the larger
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the area that was able to accumulate ice. This trend
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began at least one and a half billion years ago
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and has continued even over the past one hundred million years,
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and this suggests that ice has been building up on
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the Moon from a nearly continuous source or sources, rather
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than through a single catastrophic event such as a large
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comet or asteroid impact. For ice not only to form
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on the lunar's surface, but also to persist for hundreds
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of millions or even billions of years without evaporating, extremely
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low temperatures are required around minus one hundred and sixty
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degrees celsius, and regions that retain such cold temperatures year
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round are known as cold traps. While there are many
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permanly shadowed regions that qualifies cold traps, some do not
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because their surrounding walls can radiate heat into the crater.
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To identify the most promising regions for fighting lunar ice,
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the authors used geometric calculations. They determine which permanently shadowed
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regions also function as coal traps and when in the
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Moon's history they acquired that status. Aronson says the longer
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a given region has been a cold trap, the more
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ice it's accumulated. In most cases, a crater became shadowed
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and turned into a cold trap at the same time
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but not always. For example, Shackleton Crater has been shadowed
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for some three and a half billion years and was
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considered a promising site in the search for lunar ice,
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but Aaronson and colleagues discovered it only became a cold
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trap around half a billion years ago. To identify targets
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for future missions, the authors searched for the oldest coal
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traps and found several extensive ones more than three point
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three billion years old, located near the lunar south Pole.
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Now these findings are especially significant since locating and sampling
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lunar ice is one of the prime goals of as
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as atomis missions. Massa's long term vision includes establishing a
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permanent lunar base around twenty thirty, the surface preparation, and
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possibly a transit station for future man missions to Mass
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and beyond. Aronson says the gold standard proof for the
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existence of water ice on the Moon would be a sample.
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It would allow scientists to compare the chemical composition of
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water on the Moon with that of Earth and to
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assess whether and how manned lunar missions could make use
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of that resource. Although the origin of lunar water remains unresolved,
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scientists have built a simple mathematical model to explore various possibilities. Now,
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according to this model, the amount of ice on the
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lunar surface is affected by three processors. Water supply, evaporation,
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and what's known as impact gardening, the process in which
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it disturbance in the lunar soil and rocks redistributes ice
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and buries it beneath the surface. The observation that relatively
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little ice is found in younger colt traps, combined with
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the slow accumulation of ice over hundreds of millions of years,
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is led the authors to conclude that both water supply
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and water loss on the Moon occur at relatively rapid rates,
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like a fusst filling a leaking bucket. Now, one proposed
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source of lunar water is that volatile water from the
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Moon's interior reaches the surface through volcanic activity. Another possible
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source is the solar wind, that constant stream of charged
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particles flowing from the Sun, which includes lots and lots
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of protons. Now, when these protons hit lunar regulith, they
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can capture electrons to form hydrogen, and these same impacts
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also break chemical bonds in some regularth minerals like silicon,
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releasing oxygen atoms, which can then combine with the hydrogen
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to form hydroxyls, and these can then further bond to
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form water. A third option is the ever popular asteroid
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in comet impact, but not a single catastrophic event. Instead,
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it involved modible impacts occurring every few million years, depositing
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lots and lots of water ice. Aronson says finding water
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beyond Earth in liquid and usable form is one of
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the most important challenges in astronomy. For example, it's vital
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for life as we know it. As Earth's natural satellite,
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the Moon is an excellent laboratory for studying the history
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of our planet and its water. This report from MESSTV.
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Since the nineteen sixties, scientists have suspected that frozen water
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could survive in permanently shadowed craters at the Moon's poles.
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Both hydrogen and oxygen could be trapped within the lunar soil.
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So to find water on the Moon, scientists are looking
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for indications of hydrogen using the Lunar Reconnaissance Orbiter's Lend
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neutron detector by observing the interaction of neutrons with the
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lunar soil, scientists can interpret how much hydrogen is likely
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to be present. In order to make a detailed interpretation, however,
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LEND needs to observe a large number of neutrons. Because
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LRO is constantly moving, LEND is never over one place
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long enough to count many neutrons. So to make a
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detailed interpretation in neutron fluxed scientists add together many measurements
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from many orbits. With each orbit, LENDS data set gets
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larger and its picture of neutron flux continually improves over time.
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Places on the south pole of the Moon with the
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suppressed flux of neutrons because of their interaction with hydrogen,
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these areas strongly suggest the presence of water frozen within
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the soil. While previous lunar missions have observed indications of
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hydrogen at the Moon's south pole, the LEND measurements for
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the first time hinpoint where hydrogen and thus water is
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likely to exist. By combining years of LEND data, scientists
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see accumulating evidence that there is water on the Moon,
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and as LRO continues to return data, our picture of
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the Moon and its water will continue to get better
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in the years ahead.
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This is space time still to come, an Australian lunar
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road to land on the Moon in twenty thirty, and
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discovery of an atmosphere in a distant frozen world which
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shouldn't have one. All that and more still to come
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on space time. Nasaus slad the Australian developed Lunarova RuvA
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the flight of the Moon in twenty thirty as part
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of the Intuitive Machine CT four mission to the Luna
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South Pole. CT four will carry a squirite of six
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payloads designed to improve science's understanding of the lunar environment
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as part of NASA's Commercial Lunar Payloads Services initiative. The
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mission will fly abought the Intuitive Machines five hundred kilograms
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Nova d Lander, which is designed to deliver larger payloads
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to the lunar surface. NASAUS signed ruver with key research
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objectives including collecting new data about the local surface conditions.
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Yossi rover will be equipped with an integrated NASA payload,
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including an analysis instrument intended to demonstrate technology for scientific
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and exploration purposes. The Australian space seedbact Elo to consort him,
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which built and developed the rover, says the full mobile
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laboratory is designed to collect lunar regulars as part of
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a project to extract oxygen from the soil. Key technologies
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under development for the mission include extreme environmental robotics using
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AI and autonomous systems, the testing of new advanced sensors
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and power systems, and new communications technologies. This is space
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time still to come. Astronomers have discovered a thin atmosphere
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and a distant world far beyond Neptune with no atmosphere
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should exist, and later in the science report claims that
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both micro and nanoplastics floating in the atmosphere could be
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contributing to global warming. All that and more still to
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come on space time, astronomers to discover a thin atmosphere
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and a distant world far beyond Neptune where no atmosphere
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should exist. The tiny world, cataloged as trans Neptunian Objects
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sixty one, twenty five thirty three, two thousand and two
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XVEE ninety three, is just five hundred kilometers wide, which
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theoretically is far too small to be able to retain
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any kind of sustainable atmosphere. The findings, reported in the
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journal Nature Astronomy, raises questions about when and how the
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atmosphere on this little world. Formed. Trans Neptunian objects, or
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t and os, include thousands of small comets, icy debris,
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and frozen worlds which circle the Sun beyond the orbit
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of Neptune. A thin atmosphere has been observed around another
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trans Neptunian object, the dwarf planet Pluto, that has a
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diameter of two three hundred and seventy seven kilometers, but
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studies of other objects in the outer room of the
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Solar System have yielded negative results. That's because trans Neptunian
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objects are so called, and they're usually so small that
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their surface gravity is simply too weak they retain any atmosphere. However,
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as astronomers watched sixty one twenty five thirty three two
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thousand and two XV ninety three passed directly in front
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of or a cult at distant background star, they were
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surprised to see the star's light gradually fade rather than
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suddenly wink out, and that indicates the light was being
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attenuated as it passed through a thin atmosphere. Calculations suggest
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that this atmosphere would probably only last about one thousand
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years unless it's replenished, so that means it must have
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been created or at least replenished fairly recently. Observations by
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the James Webb Space Telescope show no signs of any
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frozen gases on the surface that might supplement to form
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an atmosphere. One possibility is that some sort of geological
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event brought frozen or liquid gases from deep inside the
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body up to its surface. Another is that a comet
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crashed into this body, releasing gases which then formed a
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temporary atmosphere. This is Space Time and Time Out of Tech.
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Another brief look at some of the other stories making
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us in science this week with a science report. A
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new study warns that micro and nanoplastics suspended in the
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air could be contributing to global warming, especially over oceanic
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garbage patches. The findings, reported in the General Nature Climate Change,
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claims the contribution of plastics is around sixteen point two
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percent of the warming effects of soot, also known as
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black carbon, and air pollutant that contributes to warming. The
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authors analyze the behavior of different plastic particles and combine
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their data with computer simulations that capture how particles travel
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in the atmosphere, finding that black and colored particles strongly
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absorb sunlight compared to white particles. Although this warming effect
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is small at the global level, it can exceed that
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of black carbon by up to alle factor of four
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