May 12, 2026
Mercury's Sulphur Secrets, Jupiter's Slimmer Profile, and NASA's Launch Tower Setback
SpaceTime Series 29 Episode 57 *How the strange magmas on Mercury shaped the planet differently to Earth A new study has found that the sulphur rich magmas on the planet Mercury reshaped the tortured world’s interior evolution and crustal formation very differently compared to the Earth. *Confirmation of a slimmer Jupiter Astronomers have revised sciences understanding of the size of the solar system’s largest planet – the gas giant Jupiter -- finding it’s some 8 kilometres narrower at the equator and 24 kilometres flatter at the poles. *Work on NASA’s Launch Tower Two formally halted NASA has issued a formal stop work order on construction of its second Mobile Launch Tower at the Kennedy Space Centre in Florida. *The Science Report Warnings the deadly H5N1 strain of bird flu can spread to humans in several different ways. Why some astronauts are at higher risk of spaceflight-associated neuro-ocular syndrome. A new study claims celebrity worship says a lot about your self-worth. Alex on Tech: warnings about streaming scams. 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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Versus Spacetime Series twenty nine, episode fifty seven, for broadcast
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in the thirteenth of May twenty six. Coming up on
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space Time, how the strange magmas on Mercury shaped the
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planet differently to the Earth, confirmation of a slimmer Jupiter,
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and work on NASA's launch tower too at the Kennedy
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Space Center has been formally halted. All that and more
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coming up on space Time.
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Welcome to space Time with Stewart Gary.
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A new study has found that sulfur rich magmas on
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the planet Mercury have reshaped the tortured world's interior, revolution
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and crustal formation very differently compared to that on Earth.
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Mercury is the nearest planet to the Sun. It's a small,
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rocky world about which scientists still know very little. Two
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missions to the planet have revealed that Mercury is covered
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by an iron pore and sulfur rich crust. Importantly, it's
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also reduced. That's a chemical state in which the substances
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have gained electrons. In fact, it's the most reduced planet
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in the Solar System. One of the studies authors, Regip
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de Scupta from the Rice Space Institute, says mercury surface
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looks completely different to that of the Earth, so scientists
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couldn't study its magmatic evolution using assumptions built on our
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understanding of the Earth. But a key to better understanding
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this distant world might come from a meteorite called indract,
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which crashed to the ground in Azerbaijan back in eighteen
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ninety one. Indract looks very similar to the chemical composition
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of mercury, and so the authors realize they could use
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it to study how mercury's unique chemical makeup shape the planet.
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That's because indract is as chemically reduced as the rocks
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on mercury. In fact, there's speculation that it may well
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have originated there. So during colleagues devolved a model melt
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composition of indract to cook their own mercury rocks in
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a high pressure, high temperature oven. The process is really
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fairly simple. Makes interacts chemical ingredients together in a small
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glass vial, change the settings in the facility to match
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the conditions on mercury, add the chemicals, and cook. This
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process of cooking a rock can show what happens chemically
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inside mercury by using the temperature, pressure, and chemical constraints
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derived both from spacecraft observations and from computer simulations. The
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authors were able to create what they believe are mercury
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like conditions in order to understand how magma's foreman evolve. There,
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they found that sulfur lowers the temperature at which these
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reduced melted rocks begin to crystallize. That means sulfur rich
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magmas on Mercury may stay molten at lower temperatures, and
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similar magmas here on Earth. Mercury's unique chemical composition, its
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low iron content, high sulfur content, and the chemically reduced
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state it's in is the reason for the significantly did
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increased crystallization temperature. Sulfur is I guess you'd call it
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a promiscuous element. It likes to be bound to other elements,
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usually iron. Iron rich planets like Mars and the Earth
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have most of their sulfur bound to iron, but Mercury's
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low iron content means its sulfur needed to find a
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different binding partner. Specifically, it could bind to major rock
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forming elements like magnesium and calcium. On Earth, these rock
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forming elements would typically bind to oxygen, resulting in a
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stable structure called a silicon network made up of silicon, oxygen,
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and rock forming elements. When sulfur replaces oxygen, however, that
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network becomes weaker and crystallizes at lower temperatures. The research
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suggests that sulfur occupies a similar structural position on Mercury
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as oxygen does on Earth, and that fundamentally changes how
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the planet's mattle solidified. There are still many questions about
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Mercury which remain to be answered, and the Joint European
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Space Agency Japan aerospacex Peration Agency BIPPI Columbo mission will
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hope to answer those when it arrives at Mercury later
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this year. This report from EAS TV.
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With a thin crust of rocks surrounding a dense iron core.
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There's more to Mercury than the first appears. Temperatures on
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the heavily cratered surface range from around four hundred and
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fifty degrees celsius down to minus one hundred and eighty,
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and there are signs of past volcanic activity. Mercury has
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been visited twice, first in nineteen seventy four by NASA's
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Mariner ten probe, and some forty years later by Messenger,
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which spent four years in orbit. Messenger mapped the surface
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and even discovered strong evidence for water ice in shaded craters.
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But the mission also raised new questions about this mysterious planet,
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questions that BEPI Columbo arbiters will be trying to answer.
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The big step forward for BEPY Columbo is the fact
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that we have two spacecraft, the European Space Agency spacecraft
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which is designed to look at the surface of the
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planet and to study the planet in detail, and the
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second spacecraft is designed to look at the environment. And
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so having two spacecraft will enable us to do a
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great deal of new science compared to the previous.
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Missions protected by the multi layered insulation, handstitched thermal blankets
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and a radiator to dissipate heat. Isa's Mercury Planetary Orbiter
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carries eleven science instruments. It will focus on studying the
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surface and internal composition of the planet.
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We will provide the three D images of the entire
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surface of Mercury and then there will be a global
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mapping with a spectrograph for the composition. It means that
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we will provide the composition within the specta range covered
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by our instrument of the entire surface of Madcur.
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A primary objective of the Japanese Mercury magnetospheric orbiters. Five
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instruments will be to study the planet's magnetic field. To
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combine data from the orbiters will enable scientists to build
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up a picture of the magnetic bubble or magnetosphere surrounding
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the planet and the influence of charged particles from the
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Sun known as the solar wind.
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With Epical on board. With a two satellite approach, we
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have one satellite, the MMO, sitting in the solar wind
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and the other one is inside the mimetosphere, so we
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can see what is coming towards the magnetosphere and what
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is driving changes within the magnetosphere.
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In that report from mes TV, we'd from Bibyklimber Mission
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scientists Emma Bunds from the University of Lister, Gabriel Criminees
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and Daniel Hayna from the Technical University of branchwag this
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space time still to came, confirmation of a slightly slimmer Jupiter,
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and Nessa formerly orders a Holt to all work and
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launch tower too at the Kennedy All that and more
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still the calm on space time well. As we reported earlier,
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a new study has now revised science as understanding of
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the size of the Solar System's largest planet, the gas
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giant Jupiter, finding it some eight kilometers narrow at the
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equator and twenty four kilometers flatter at the poles. The
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new confirmation, reported in the journal Nature Astronomy, measured Jupiter's
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dimensions with unprecedented precision. For more than fifty years, astronomers
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thought they knew the size and shape of Jupiter based
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on six measurements made by NASA's Voyager and Pioneer spacecraft.
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The studies lead author Eli Glente from Israel's Weismann Institutes
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is These original measurements were based on radio signals sent
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from the spacecraft back to Earth. Glenty says those missions
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provided a foundation, but now scientists can use data from
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as many as twenty six measurements made thanks to NASA's
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Juno spacecraft. Just by knowing the distance to Jupiter and
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watching how it rotates allows scientists to figure out roughly
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its shape and size, but making really accurate measurements calls
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for far more sophisticated methods. Launched in twenty eleven and
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orbiting Jupiter since twenty sixteen, Juno has been sending streams
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of raw data back to Earth. When NASA extended the
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mission in twenty twenty one, the spacecraft was able to
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keep studying Jupiter and its moons more closely, and juno's
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new expanded path placed the spacecraft in an orbit that
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allowed it to pass behind Jupiter from Earth's point of view,
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something its earlier orbit couldn't do, and JUNO passing behind
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Jupiter provides an opportunity for use science objectives. When the
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spacecraft passes behind the planet, its radio communications signal is
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blocked and bent by Jupiter's atmosphere. Juno's principal investigator, Scott
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Bolton from the Southwest Resil Institute in San Antonio, Texas,
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says this enables a more accurate measurement of Jupiter size.
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The JUNO team at the Weisman Institute seized on the
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new opportunity and tracked how the radio signals bent as
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they passed through Jupiter's atmosphere. This allowed the authors to
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translate this information into detailed maps of Jupiter's temperature and density,
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producing the clearest picture yet of the giant planet size
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and shape. The new findings show the King of Planets
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is far more flattened that the poles compared to previous estimates,
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and Galati says those few kilometers matter because shifting the
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radius by just a little let's models of Jupiter's interior
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fit both the gravity data and atmospheric measurements far better.
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This implication was then tested using models for the interior
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density structure of Jupiter to show that the refined shape
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helps bridge the gap between the models and the measurements.
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The study also has broader implications for understanding the structure
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of gas planets in general. That's because Jupiter serves as
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a standard reference for the study of gas giants both
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within our Solar System and beyond, and the earlier measurements
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didn't account for Jupiter's powerful winds. By including these extreme
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winds in their calculations, the authors cleared up some long
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standing discrepancies in earlier measurements. It's difficult to see what's
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happening beneath those swirling clouds of Jupiter, but the radio
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data is giving scientists to window into the depth of
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Jupiter' zonal winds and powerful hurricanes, and the work on
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the winds ties in with a recent study of Jupiter's
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vast polar cyclones. That research used generous measurements of these
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cyclones motions to predict how deep into the interior they extend. Overall,
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and improved understanding of Jupiter's winds enabled scientists to better
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understand the relationship between the planet's atmosphere and its deep interior.
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This space time still to come. NASAs issued a formal
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stop work order on construction of its second mobile launched tower,
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and later in the science report warnings the deadly H
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five and one strand of bird flu has found new
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ways to infect humans. All that and more still to
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come on space time, NASA is issued a formal stop
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work order on construction of its second mobile launch tower
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at the Kennedy Space Center in Florida. The move comes
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in the wake of the agency's decision to continue with
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the existing Space Launch System SOLS rocket in only its
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current Block one form rather than proceed with a larger
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Block one B in Block two versions. The second mobile
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launch tower would have been needed to handle the taller
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SLS Block one B in Block two, which would have
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used the bigger four engine Exploration upper stage rather than
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the single engine interim cryogenic propulsion stage which is used
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on the SOLS Block one. The interim cryogenic propulsion stage,
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which was only ever intended for use in the Atomus one, two,
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and three missions, was based on the second stage of
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the Narra tired Delta four rocket, and so production has
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been shut down. The original plans called for Atoms four
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onwards to use the more powerful Specially develop Exploration upper stage,
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but with that program canceled allegedly to standardize the SLS design,
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NASA will now instead switched to a two engine cent
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or five upper stage based on that currently used on
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the United launch a lines Vulcan rocket, as well as
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being two meters taller and fitted with repositioned umbilicals for
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the expiration upper stage. The second mobile launch tower is
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also structurally stiffer and more than three meters wider in
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order to handle the bigger loads which were planned for
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the now defunct Block one B and Block two versions.
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NASA says it will now start stripping parts off the
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second launch tower for use of spares on Tower one.
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The agency says the second mobile launch tower was too heavy,
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it was years late, and it was pushing close to
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a billion US dollars in costs. This is base time
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and Time Out of Tech. Another brief look at some
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of the other stories making news in Science this week
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with a science report. A new study has shown how
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the deadly H five N one strand of bird flu
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can spread between dairy cattle and humans using several different paths,
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not just through exposure to contaminated milk. The findings, reported
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in the journal Plus Biology, based on air, farm water,
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and milk samples from fourteen dairy farms, which all tested
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positive for H five one across two regions of California.
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The authors detected the virus in the air from the
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ex hooured breadth of infected cows in milking sheds, as
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well as in wastewater from those sheds, and they also
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found many cows that tested positive for H five N
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one despite not showing any symptoms. The findings highlight the
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sheer matter of the virus now circulating on infected farms
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and the range of ways in which H five H
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one infection can spread between cows and people. The authors
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say providing cleaner air in milking sheds and ensuring any
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milk from infected animals is properly disposed of could cut
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the risk of this deadly bird flues spreading. Scientists have
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used data from the lifetime surveillance of Astronaut Health Program,
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together with measurements of vision and eye health both before
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and after spaceflight to determine which astronauts are most likely
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to develop spaceflight associated neuro ocular syndrome. The condition includes
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changes in both long and short sightedness, the loss of
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the eyes around shape at the back, the development of
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wrinkles or lines at the very back of the eye,
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and optic disc edema, where the spot at the back
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of the eye where the optic nerve connects squells up.
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A report in the Journal of the American Medical Association
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found body mass index was the strongest predictor of whether
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an astronaut will experience this problem, and those carrying more
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weight were at greater risk. Now this may be because
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weightlessness changes the amount of pressure in the eye, and
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these effects are therefore more pronounced among people who are heavier.
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A new study claims celebrity worship says a lot about
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a person's self worth. In today celebrity and influencer driven culture,
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psychologists are increasingly interested in why people form strong emotional
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connections with certain famous figures. The new research, reported in
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the journal Personality and Individual Differences, suggest that celebrity admiration
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is closely linked to how clearly people understand themselves. The study,
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