WEBVTT

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Anna: Welcome to Astronomy Daily, your regular dose

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of cosmic insights with your host, Anna.

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Today, we're diving into how a massive

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ancient impact shaped our planet for life,

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uncovering new secrets about ice and space,

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and getting the latest on exciting space

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missions and rocket launches. Plus, we'll

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guide you through observing, uh, July's

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beautiful Buck Moon and commemorating a

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historic lunar anniversary. Let's get started

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with a story about our home planet.

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Earth, alone among the rocky planets in our

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solar system, is a vibrant home for life.

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It's warm, hospitable and teeming with

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activity, a stark contrast to the frigid

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lifelessness of its neighbours. How did our

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planet become so uniquely suited for life?

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The answer is incredibly complex. But a

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significant part of it lies in the

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fascinating field of cosmochemistry, which

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explores how chemical elements are

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distributed across the cosmos. Imagine

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our solar system. 4.5 billion years ago,

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it was a far more chaotic place than it is

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today, with planets still in their infancy

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and countless planetesimals and planetary

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embryos whizzing around constantly crashing

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into each other. Amidst this

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cosmic demolition derby, something

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extraordinary happened. Earth somehow

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received an exceptionally generous delivery

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of carbonaceous chondrites. These

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aren't just any space rocks. They're packed

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with amino acids and other essential

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chemicals, the very building blocks that

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enable life. Cosmochemistry studies have

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revealed that between 5 and 10% of Earth's

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entire mass originated from these

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carbonaceous chondrites that collided with

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our young planet. What's even more astounding

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is that a substantial portion of this life

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enabling material is believed to have arrived

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during the colossal impact, eventually that

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formed our moon. The THEIA impact.

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To rigorously test this profound idea, a

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team of researchers led by Duarte Branco

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from the Institute of Astrophysics and Space

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Sciences in Portugal, utilised sophisticated

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dynamical simulations of the solar

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system's formation. Their groundbreaking

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work, titled Dynamical Origin of Theia uh,

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the Last Giant Impactor on Earth, is set to

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be published in the journal IT icarus.

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In cosmochemistry, a critical distinction is

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made between carbonaceous chondrites, or ccs,

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and non carbonaceous meteorites.

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This effectively divides the solar system's

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meteorite population into two distinct

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material reservoirs. Ccs formed much

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farther from the sun, likely beyond Jupiter,

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and are rich in volatiles like water and

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organic compounds. Ncs, on the other

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hand, include things like iron meteorites and

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contain far fewer volatile elements. The

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core question for the researchers was whether

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Theia uh, could have delivered these crucial

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CCS and volatiles to early Earth.

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To investigate this, the team ran detailed N

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body simulations focusing on the later stages

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of terrestrial planet growth, specifically

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after the solar system's gaseous disc had

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dissipated. These simulations included

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CCs that were scattered inward as gas giants

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like Jupiter and Saturn were still growing.

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The researchers explored three main

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scenarios, one with only small CC

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objects or planetesimals, another with only

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large CC objects or planetary embryos, and

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a mixed scenario that included both.

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A subset of these simulations also factored

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in the giant planet dynamical instability,

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better known as the NICE model in astronomy.

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This model describes how the giant planets

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shifted their orbits from their initial

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formation positions. The goal was

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multifaceted to understand how ccs and

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ncs were distributed, why Earth ended up with

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significantly more ccs than other rocky

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planets, particularly Mars, and whether the

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Theia impact was indeed responsible for

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delivering a large amount of Earth's C C

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material. One of the most striking results

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showed that the giant planet instability,

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especially Jupiter's orbital shift, had a

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profound effect on Earth's accretion of C C

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material. As the giant planets moved,

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they caused a strong pulse of eccentricity

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excitement, leading to a wave of collisions

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and ejections, effectively flinging CC rich

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material into the inner solar system.

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Crucially, the simulations strongly supported

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the idea that THEIA itself was a carbonaceous

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object. In the mixed scenario simulations

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without giant planet instability, Earth's

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final impactor, Theia, included a

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carbonaceous component in more than half of

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all simulations. In 38.5%

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of cases, Theia was a pure carbonaceous

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embryo, and in another 13.5%,

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it was an NC embryo that had previously

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accreted a C C embryo. This paints a

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vivid picture of the early solar system. Two

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distinct rings of planetesimals, an inner

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ring of rocky material and an outer ring of

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carbonaceous chondrites. As uh, the ice

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giants migrated inward, they propelled this

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CC material into the inner solar system, with

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more massive ones preferentially scattered

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into the orbits of rocky planets. This

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explains not only the masses and orbits of

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the terrestrial planets and the distribution

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of asteroids, but also why Earth has a higher

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CC mass fraction compared to Mars. The work

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strongly suggests that Earth's final giant

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impact was indeed with Theia, and that this

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object had a higher concentration of

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carbonaceous material directly contributing

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to our planet's habitability. The

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simulations indicate this last impact

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occurred between 5 and 150-million years

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after the gas disc dispersed, with a large

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fraction happening within 20 to 70 million

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years, timings consistent with current

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understanding of the Theia impact. Moreover,

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the research emphasises Jupiter's pivotal

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role in shaping the solar system's

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Architecture not just by truncating the

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asteroid belt, but also by scattering crucial

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carbonaceous material from the outer solar

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system into the path of the rocky planets,

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especially Earth. Ultimately, the

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formation of a life sustaining world like

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Earth required an astonishing number of

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variables to align perfectly. This research

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highlights that it may take more than simply

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being in a habitable zone for an exoplanet to

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support life. The complex dance of outer

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giant planets migrating and delivering carbon

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to inner rocky worlds might be another

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critical, often overlooked ingredient in the

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recipe for life in the universe.

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Alright, moving on. Prepare to have your

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perceptions of space ice completely

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shattered. For decades, scientists have

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largely viewed water frozen in the depths of

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space as a shapeless, amorphous fog. Too

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cold and still to ever form orderly crystals,

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it was believed to simply freeze straight

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from vapour onto cold surfaces like dust

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grains and comets or icy moons without any

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structured shape whatsoever. But a

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groundbreaking new study by researchers from

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University College London and the University

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of Cambridge is challenging that long held

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belief. By combining incredibly detailed

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computer simulations with carefully

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controlled lab experiments, this team has

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discovered that space ice is not entirely

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amorphous after all. Instead, it holds

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tiny hidden crystal structures within its

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disordered form. These small organised

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patterns could fundamentally shift what we

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know about ice, water and even the very

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origins of life in the universe. On Earth,

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ice typically forms a neat crystalline

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pattern visible in the intricate symmetry of

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a snowflake. But in the extreme cold and

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vacuum of interstellar space, we where

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temperatures plummet far below freezing. It

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was thought that ice formed without any

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order. This form of water was known as low

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density amorphous ice, and the prevailing

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view was that it lacked any internal

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structure. However, that view is now

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rapidly changing. The researchers began

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by freezing virtual boxes of water molecules

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down to an incredibly chilly negative

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120 degrees Celsius. This allowed them

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to simulate how ice forms at various rates.

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Some simulations indeed produced nearly

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perfect disordered ice. But others revealed

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something fascinating. Tiny crystals

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roughly 3 nanometers wide that's just

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slightly larger than a strand of DNA, began

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to form within the chaos. The result that

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most accurately matched existing X ray

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diffraction data wasn't fully disordered ice.

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Instead, it was found to be approximately 20%

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crystalline and 80% amorphous.

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Dr. Michael B. Davies, the lead author of

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this pivotal study, noted, we now have a

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good idea of what the most common form of ice

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in the universe looks like at an atomic

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level. He emphasised the importance of this

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finding, explaining that ice is involved in

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many cosmological processes, for instance, in

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how planets form, how galaxies evolve,

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and how Matter moves around the universe.

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The team didn't stop at simulations. They

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meticulously created real samples of

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amorphous ice in their lab using several

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methods. One method directly mimicked how

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ice forms in space by depositing water

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vapour onto a surface chilled far below

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freezing. Another involved crushing normal

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ice at very low temperatures to produce high

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density amorphous ice. After creating

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both types, the researchers carefully warmed

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the samples, allowing crystals to develop.

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Here's where it got even more interesting.

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They observed that each sample produced a

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different crystal pattern once it warmed.

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This was a critical observation. If the ice

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had truly been fully amorphous, completely

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without any order, it shouldn't have retained

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any memory of its earlier form. But

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because it did, the scientists concluded that

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even space ice, despite its seemingly

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shapeless appearance, retains some hidden

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structure within. As Professor Christoph

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Salzman, a co author of the study, put it,

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ice can remember its previous structure. The

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order of hydrogen atoms in a crystalline

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state can be preserved even as conditions

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change. This suggests that space ice is far

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more complex than previously thought,

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carrying clues about its origin and the

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environment in which it formed. These

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findings have significant implications,

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particularly for theories regarding the

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origin of life beyond Earth. One prominent

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theory, known as panspermia, suggests that

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life's essential ingredients, such as amino

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acids, may have arrived on Earth from space,

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perhaps carried by comets. This idea

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relies on space ice being able to effectively

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trap and protect complex molecules during

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their long journeys across the cosmos.

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However, this new discovery complicates that

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idea slightly. As Dr. Davies

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explained, our, uh, findings suggest this ice

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would be a less good transport material for

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these origin of life molecules. That is

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because a partly crystalline structure has

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less space space in which these ingredients

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could become embedded. While this might

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weaken the panspermia argument slightly, it

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doesn't rule it out entirely. Davies added

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that the theory could still hold true, as

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there are amorphous regions in the ice where

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life's building blocks could be trapped and

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stored. Ultimately, these

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results provide a more realistic picture of

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the conditions life's precursors might

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encounter while travelling through the vast

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emptiness of space. The implications of this

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research extend far beyond just the origin of

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life. Amorphous materials are incredibly

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common in modern technology. For example, the

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glass used in fibre optic cables, which

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transmit data across the globe, must remain

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in a disordered state for optimal

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performance. If these materials contain tiny

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hidden crystals that could affect their

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performance, understanding how to remove them

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could lead to significant advancements and

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better technology. Professor Saltzman

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also highlighted this, stating,

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our results also raise questions about

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amorphous materials. In general, these

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materials have important uses in much

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advanced technology. If they do contain tiny

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crystals and we can remove them, this will

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improve their performance. Furthermore,

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this knowledge could help space agencies

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design more effective spacecraft. Ice in

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space isn't just a passive substance. It has

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the potential to serve as radiation shielding

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or even as a source of fuel. If broken down

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into hydrogen and oxygen. Knowing more about

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its various forms and structural properties

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could lead to smarter and more efficient uses

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for this vital cosmic resource. As Dr.

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Davies noted, ice is potentially a high

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performance material in space. It could

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shield spacecraft from radiation or provide

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fuel in the form of hydrogen and oxygen. So

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we need to know about its various forms and

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properties.

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Next up today, let's take a look at launch

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plans. As you well know, we're

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constantly looking to the future in space,

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and some truly ambitious plans are on the

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horizon. Chinese scientists have put forward

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a fascinating proposal for the country's very

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first ice giant mission. Their goal is to

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launch a radioisotope powered spacecraft by

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2033, destined to orbit

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Neptune and conduct an in depth study of its

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mysterious moon Triton. This

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mission promises to shed new light on one of

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the most distant and least understood worlds

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in our solar system. Closer to home, it's

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been a bustling period for rocket launches.

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Even in what was described as a quiet week

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for orbital flights, SpaceX

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recently achieved a monumental milestone,

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completing the 500th orbital flight of its

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workhorse Falcon 9 rocket launchers. This

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incredible feat was part of their Starlink

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Group 1028 mission, which lifted off from

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Cape Canaveral Space force station. The

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Falcon 9 has certainly earned its reputation,

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celebrating over 15 years since its

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inaugural flight in June 2010.

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This 500th launch saw Booster

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B1077 make its 22nd

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flight, a testament to the reusability

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pioneered by SpaceX. With the Booster aiming

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for its 490th recovery attempt on the drone

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ship, a shortfall of gravitas in late

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June, SpaceX also set new records with back

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to back launches from Florida and California,

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marking their 80th and 81st Falcon missions

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of the year. They even achieved a new pad

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turnaround record of just over 56 hours at

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Space Launch Complex 40. This

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relentless pace has contributed to a

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significant increase in global launch

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cadence, with 142 orbital launches

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worldwide in the first half of the year, a

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16% jump compared to 2024.

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Keep an eye out as another Falcon 9 launch is

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anticipated soon, possibly carrying the

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Israeli Dror 1 communications satellite into

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geostationary transfer orbit.

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Meanwhile, on the other side of the world,

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Australia is gearing up for a historic moment

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in its space programme. Gilmour Space

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is preparing for the highly anticipated

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maiden launch of its Eris small satellite

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rocket. This will be their second attempt

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after the previous one in May was postponed

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due to a power surge that prematurely

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triggered the fairing separation system, an

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issue that has since been successfully

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mitigated. The Eris rocket is set

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to lift off from the Bowen Orbital Spaceport

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at Abbott Point, making it the first orbital

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launch from Australian soil performed by a

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sovereign built vehicle. Standing at 25

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metres tall and boasting a payload capacity

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of up to 215 kilogrammes to a 500

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kilometre sun synchron orbit, Eris is

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comparable in size and capability to Rocket

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Lab's Electron. Its first stage is propelled

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by four proprietary Sirius Hybrid engines

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which use a unique 3D printed solid fuel

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grain and hydrogen peroxide as the

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oxidizer. A successful orbital launch would

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also mark a significant first for a hybrid

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rocket design showcasing a new frontier in

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propulsion technology.

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Now let's turn our gaze to the night sky,

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because July 2025 promises a spectacular

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lunar event. The Full Moon, affectionately

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00:15:39.670 --> 00:15:42.190
known as the Buck Moon, is set to rise on

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Wednesday, July 10. This celestial display is

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perfect for both seasoned stargazers and

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00:15:47.110 --> 00:15:49.910
budding astrophotographers. A full

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moon occurs when our moon is perfectly

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positioned opposite the sun in the sky,

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allowing it to appear completely

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illuminated from our perspective here on

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Earth. The Buck Moon gets its

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00:16:02.470 --> 00:16:04.870
evocative name from the time of year in North

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00:16:04.870 --> 00:16:07.480
America when male deer or bucks

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00:16:07.720 --> 00:16:09.600
are actively growing out their impressive

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00:16:09.600 --> 00:16:12.240
antlers. It's also sometimes referred to as

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00:16:12.240 --> 00:16:14.600
the Thunder Moon, a nod to the frequent

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00:16:14.600 --> 00:16:16.640
summer storms that rumble across parts of the

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US In July this year. The Buck

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Moon holds another distinction. It arrives

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00:16:21.719 --> 00:16:23.440
less than a week after Earth reaches

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00:16:23.440 --> 00:16:26.240
aphelion, its farthest point from the sun in

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its orbit, making it the most distant Full

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00:16:28.600 --> 00:16:31.530
Moon from the sun in 2025. While the

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00:16:31.530 --> 00:16:33.730
Moon technically reaches its fullest phase at

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00:16:33.730 --> 00:16:36.210
4:36pm Eastern Daylight Time

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00:16:36.610 --> 00:16:39.570
or 20:36 GMT on July 10,

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it won't be visible to us until it rises

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00:16:41.930 --> 00:16:44.330
above the southern horizon at sunset in your

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00:16:44.330 --> 00:16:47.089
local time zone. For instance, if

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00:16:47.089 --> 00:16:48.570
you're in New York City, you can expect

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00:16:48.570 --> 00:16:51.330
moonrise around 8:53pm local time.

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00:16:51.890 --> 00:16:54.210
Remember that exact timings for moon phases

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00:16:54.210 --> 00:16:56.850
can vary depending on your location, so it's

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00:16:56.850 --> 00:16:58.770
always a good idea to check a trusted website

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00:16:58.770 --> 00:17:01.490
like in the sky.org or timeanddate.com for

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00:17:01.490 --> 00:17:04.400
precise local timings. You might notice

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00:17:04.400 --> 00:17:06.320
something particularly striking about July's

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00:17:06.320 --> 00:17:09.040
Full moon. It will appear exceptionally low

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00:17:09.040 --> 00:17:11.960
in the sky after sunset. This phenomenon is

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00:17:11.960 --> 00:17:13.920
largely due to its proximity to the summer

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00:17:13.920 --> 00:17:16.200
solstice, the time when the sun is at its

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00:17:16.200 --> 00:17:17.960
highest point in the daytime sky.

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00:17:19.080 --> 00:17:20.760
Consequently, the Moon tracks a

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00:17:20.760 --> 00:17:23.000
correspondingly low path through the night.

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00:17:23.320 --> 00:17:26.080
This effect is even more pronounced in 2025

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00:17:26.080 --> 00:17:28.480
thanks to a fascinating occurrence known as a

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00:17:28.480 --> 00:17:31.110
major lunar standstill. This happens

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00:17:31.110 --> 00:17:34.110
approximately every 18.6 years when the

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00:17:34.110 --> 00:17:36.590
Sun's gravity influences the Moon's tilted

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00:17:36.590 --> 00:17:38.790
orbit, pushing it to its most extreme

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00:17:38.790 --> 00:17:41.110
inclination relative to Earth's celestial

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00:17:41.110 --> 00:17:44.030
equator. This orbital dance causes the Moon

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00:17:44.030 --> 00:17:46.670
to appear either exceptionally high or, as in

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00:17:46.670 --> 00:17:49.230
this case, notably low in our sky, depending

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00:17:49.230 --> 00:17:51.950
on the time of year. As you observe the

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00:17:51.950 --> 00:17:54.270
Buck Moon, especially in the hours following

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00:17:54.270 --> 00:17:57.270
moonrise on July 10, you might experience a

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00:17:57.270 --> 00:17:59.830
common optical illusion, the Moon

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00:17:59.830 --> 00:18:02.470
illusion. This is when the lunar disc

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00:18:02.470 --> 00:18:04.950
appears larger than it actually is when it's

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00:18:04.950 --> 00:18:07.750
positioned close to the horizon. Our

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00:18:07.750 --> 00:18:09.710
brains, for reasons still debated by

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00:18:09.710 --> 00:18:12.070
scientists, trick us into thinking it's

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00:18:12.070 --> 00:18:13.670
bigger than it appears when directly

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00:18:13.670 --> 00:18:16.390
overhead, even though its actual size in the

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00:18:16.390 --> 00:18:19.230
night sky remains constant. You might also

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00:18:19.230 --> 00:18:21.150
notice the Buck Moon take on a beautiful

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00:18:21.150 --> 00:18:23.790
golden or reddish hue shortly after it rises.

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00:18:24.350 --> 00:18:26.510
This warm coloration is caused by Rayleigh

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00:18:26.510 --> 00:18:28.870
scattering, the very same atmospheric effect

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00:18:28.870 --> 00:18:31.030
that paints our sunsets and sunrises with

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00:18:31.030 --> 00:18:33.590
vibrant colours. When the moonlight reflected

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00:18:33.590 --> 00:18:35.590
off the Moon's surface travels through more

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00:18:35.590 --> 00:18:37.590
of Earth's atmosphere to reach us at the

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00:18:37.590 --> 00:18:40.590
horizon, the shorter, bluer wavelengths

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00:18:40.590 --> 00:18:42.910
of light are scattered away, allowing the

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00:18:42.910 --> 00:18:45.030
longer, redder wavelengths to pass through

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00:18:45.030 --> 00:18:47.750
more directly beyond the enchanting

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00:18:47.750 --> 00:18:50.280
display of the Buck Moon. The this month also

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00:18:50.280 --> 00:18:52.760
marks a significant anniversary in human

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00:18:52.760 --> 00:18:55.160
spaceflight history. The 56th

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00:18:55.160 --> 00:18:57.960
anniversary of the Apollo 11 moon landing.

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00:18:58.600 --> 00:19:01.480
On July 20, 1969, Neil

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00:19:01.480 --> 00:19:03.640
Armstrong and Buzz Aldrin became the first

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00:19:03.640 --> 00:19:06.080
humans to walk on the Moon, while Michael

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00:19:06.080 --> 00:19:08.800
Collins expertly orbited above. To

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00:19:08.800 --> 00:19:11.000
commemorate this incredible achievement, we

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00:19:11.000 --> 00:19:13.400
invite you to try and locate the six historic

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00:19:13.400 --> 00:19:15.770
Apollo era landing sites on on the lunar

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00:19:15.770 --> 00:19:18.530
surface. With the naked eye, you can

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00:19:18.530 --> 00:19:21.010
often spot the general region visited by each

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00:19:21.010 --> 00:19:23.970
Apollo mission, but if you have access to a 6

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00:19:23.970 --> 00:19:26.570
inch telescope, it will greatly enhance your

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00:19:26.570 --> 00:19:29.530
viewing experience, helping to reveal finer

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00:19:29.530 --> 00:19:31.970
details in the rugged moonscapes and smooth

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00:19:31.970 --> 00:19:34.290
lunar seas surrounding each of these historic

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00:19:34.290 --> 00:19:36.850
zones. It's a wonderful way to connect with a

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00:19:36.850 --> 00:19:38.890
pivotal moment in our shared human journey of

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00:19:38.890 --> 00:19:39.570
exploration.

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00:19:41.410 --> 00:19:43.450
That's all for this episode of Astronomy

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00:19:43.450 --> 00:19:45.370
Daily. We hope you enjoyed our journey

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00:19:45.370 --> 00:19:47.890
through cosmic origins, the secrets of space

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00:19:47.890 --> 00:19:50.730
ice, and the latest in space exploration and

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00:19:50.730 --> 00:19:53.330
sky watching. A quick reminder before I log

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00:19:53.330 --> 00:19:56.250
off Visit Astronomy Daily IO to sign

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00:19:56.250 --> 00:19:58.530
up for our free daily newsletter and explore

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00:19:58.530 --> 00:20:01.210
all our back episodes. Remember to subscribe

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00:20:01.210 --> 00:20:03.370
to Astronomy Daily on Apple Podcasts,

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00:20:03.370 --> 00:20:05.850
Spotify, YouTube, or wherever you get your

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00:20:05.850 --> 00:20:08.250
podcasts. Until tomorrow, this is Anna

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00:20:08.250 --> 00:20:10.330
reminding you to keep looking up and

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00:20:10.330 --> 00:20:12.250
marvelling at our wonderful universe.
