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Anna: Welcome to Astronomy Daily. I'm your host,

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Anna, and I'm thrilled you're joining us for

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another exciting dive into the cosmos.

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Today we'll be exploring the recent

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challenges faced by some ambitious

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spacecraft, uncovering surprising new

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discoveries about our very own Milky Way

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galaxy, and discussing a potential hidden

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family of asteroids that might be sharing

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Venus's orbit. Plus, we'll take a look

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ahead at what promises to be a very busy week

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for space launches around the globe. Stay

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with us. First up,

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let's talk about the challenges of lunar

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exploration.

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Japanese company ISPACE has announced that it

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believes its second lunar lander mission,

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named Resilience, crashed due to problems

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with its laser rangefinder. This crucial

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piece of equipment is designed to determine

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altitude during descent, but it reportedly

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suffered a hardware issue. During a press

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briefing, company executives explained that

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the laser rangefinder, meant to provide the

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first altitude data at 3 km above the

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surface, didn't give its initial measurement

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until the lander was less than 900 meters

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high. By then, the spacecraft was

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traveling much faster than planned, reaching

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66 meters per second compared to the

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intended 44 meters per second. The last

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telemetry from the lander at an altitude of

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192 meters, still showed it descending

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rapidly at 42 meters per second.

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Images later released by NASA's Lunar

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Reconnaissance Orbiter show a 16 meter wide

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crater marking the probable crash site.

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ISpace's executive vice president

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Yoshitsugu Hitachi clarified that this

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incident was different from their first

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mission in 2023, which failed due to

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a software error. While the software on

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Resilience worked as intended, the laser

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rangefinder was a different model but sourced

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from a new unnamed supplier.

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Investigations ruled out improper

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installation, leading the company to conclude

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the unit's performance simply degraded.

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Several factors could have caused this,

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including lunar surface conditions, reduced

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laser power, or even effects from the space

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environment like vacuum and radiation.

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Looking ahead, ISPACE is taking significant

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steps to prevent future issues. Chief

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Technology Officer Ryo Ujiya stated they will

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enhance testing for the laser rangefinder and

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and related sensors to better simulate high

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speed and low reflectivity conditions.

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They're also considering using a different

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flight proven laser rangefinder and

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augmenting it with other sensors like LIDAR

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or cameras for more robust navigation.

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These efforts will be supported by a new

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external review board, including former

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engineers from NASA and the Japanese space

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agency jaxa. Despite the setbacks,

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ISPACE remains committed to, with CEO

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Takeshi Hakamada emphasizing their resolve

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to keep improving and moving forward with

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their next missions, both still scheduled for

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2027.

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Moving on let's turn our attention to Europe,

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where the exploration company recently faced

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a setback with its Mission Possible Test

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vehicle. This European company, which

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aims to develop orbital spacecraft for cargo

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and eventually human transport, achieved a

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partial success and a partial failure in

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its latest test flight. The vehicle

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powered up and flew successfully in orbit

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before making a controlled RE entry into

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Earth's atmosphere. Crucially, it

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managed to re establish communication after

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the blackout period, suggesting it navigated

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the most thermally challenging part of

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reentry effectively. However, the company

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lost contact with the spacecraft just a few

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minutes before its planned touchdown in the

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ocean. In a candid update, the

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exploration company indicated that the most

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likely culprit was an issue with the

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deployment of its parachutes, which were

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designed to deploy at specific velocities

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during descent. This demonstration

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vehicle, measuring two and a half meters in

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diameter, aimed to test four key

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structural performance in orbit, surviving RE

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entry, autonomous navigation, and recovery in

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real world conditions. It only clearly failed

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in this final critical task of recovering the

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vehicle M. Despite this challenge, the

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company's transparent and rapid communication

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acknowledging the partial failure within

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hours of the launch is quite refreshing in

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the space industry. The Mission Possible

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vehicle was developed at a relatively low

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cost of about $20 million in just

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2.5 years, demonstrating

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the company's aggressive timeline and

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commitment. While it's possible the

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exploration company might conduct another

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subscale demonstration, this mission

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represents a significant step forward for

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Europe's commercial space sector, which has

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historically lagged behind the US And China.

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The ability to launch a fairly large vehicle

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and bring it back through Earth's atmosphere

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less than four years after the company's

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founding is a credible and promising start.

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They are now focused on developing their full

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size Nix cargo spacecraft with a potential

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flight as early as 2028.

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Now let's shift our gaze closer to home

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within our own cosmic neighborhood.

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Astronomers have recently developed a

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groundbreaking new method for accurately

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mapping the outer gas disk of the Milky Way,

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and what they've found is quite surprising.

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It turns out our galaxy's structure is far

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more complex than previously thought,

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complete with what they describe as

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flocculant or tufty looking gas clouds.

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This innovative approach, pioneered by

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Sukanya Chakrabarti of the University of

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Alabama and Peter Craig from msu,

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relies on determining the precise distances

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to very young stars within the outer disk.

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They leverage data from the European Space

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Agency's Gaia satellite, which has

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meticulously measured the brightness,

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positions, motions, and, crucially, the

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distances to nearly 2 billion Milky Way

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stars. As Chakrabarti emphasized,

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distance is one of the most Fundamental

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things you can measure in the universe.

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Unless you know distances, you can't map

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anything. This is a significant departure

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from traditional mapping methods that use

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kinematic distances which assume a model for

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the galaxy's velocity fields. These

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older methods can be imprecise, especially

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for gas clouds which appear much fleecier and

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more disturbed than the smoother patterns

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seen in stars. To overcome these

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inaccuracies, the team used a clever pattern

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matching technique. They observed that the

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spiral structure in the gas clouds of nearby

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galaxies closely mirrors the structure of

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young stars less than 400 million years old,

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which are born from these gas clouds. By

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pairing young stars with known locations to

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nearby clumps of gas, they created a new map

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that isn't dependent on the problematic

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kinematic assumptions. For highly accurate

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distance markers, they relied on Cepheid

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variable stars which pulsate with a, uh,

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regular rhythm, allowing astronomers to

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calculate incredibly precise distances.

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The results are transforming our

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understanding. Craig noted that their new

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maps nicely demonstrate that the spiral

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structure in the gas disk of the Milky Way is

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highly flocculant and that the overall

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structure of the disk is complex. This

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technique combining pattern matching with

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accurate stellar distances promises to

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significantly improve our understanding of

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the prevalence and shapes of the clouds in

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the hydrogen disk. Beyond that,

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these more accurate maps can enhance three

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dimensional dust maps of the entire galaxy

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and help astronomers identify disturbances

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within the disk, such as interactions with

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nearby dwarf galaxies or even the presence

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of dark matter. It's a truly exciting

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development that paints an even more

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intricate picture of our home galaxy

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moving from the intricate patterns within our

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own Milky Way.

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Let's turn our attention to an exciting

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discovery much closer to home, right in our

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solar system. Astronomers are currently

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delving into a little known and largely

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unseen group of asteroids that quietly share

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Venus's orbit around the Sun. These

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fascinating space rocks, dubbed Venus Co

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orbital asteroids, might be far more numerous

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than we ever imagined. To date, only

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about 20 of these unique asteroids have been

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confirmed. However, a new study led by

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Valerio Carruba from Sao Paulo State

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University in Brazil the suggest that

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hundreds more could be lurking just out of

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sight. Karuba excitingly compared this

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potential discovery to discovering a

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continent you didn't know existed. The reason

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so few have been found until now is their

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elusiveness. They appear close to the sun in

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our sky, making them difficult for ground

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based telescopes to spot. And their rapid

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movement adds to the tracking challenge.

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To investigate this hidden population,

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Karuba's team ran extensive computer

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simulations modeling the orbits of hundreds

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of hypothetical Venus Co orbital asteroids

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over a staggering 36,000 years into

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the future, they found that many of these

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objects could remain gravitationally bound to

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Venus's orbit for an average of about 12,000

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years. Interestingly, their orbits appeared

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chaotic, meaning small shifts over long

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periods could eventually push them onto

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different paths, including some that might

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bring them closer to Earth. However, there's

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no need for alarm. Experts, including

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astronomer Scott Shepard from the Carnegie

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Institution for Science, emphasize that none

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of the known asteroids pose an immediate

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threat, and the timescales involved span many

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thousands of years. The likelihood of one

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colliding with Earth anytime soon is

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extremely low. Despite the low risk,

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understanding these objects is crucial for

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building a more complete picture of near

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Earth space. Because they're so hard to spot

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from Earth, the team also explored new

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detection methods. Their simulations suggest

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that a spacecraft orbiting closer to Venus

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would have a much better chance. And the

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newly commissioned Vera C Rubin Observatory,

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though not specifically designed for the

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inner solar system, could potentially catch

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some of these hidden asteroids during its

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special twilight observing campaigns. Further

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into the future, a proposed mission concept

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called Crown and envisions a fleet of small

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spacecraft near Venus specifically designed

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for this search. These efforts promise to

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unveil many more of these dynamically

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intriguing objects, adding another layer to

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our understanding of the solar system's

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diverse inhabitants.

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From hidden asteroids to perplexing planets,

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astronomers have been busy unraveling cosmic

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mysteries. And speaking of mysteries,

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scientists may have finally cracked the

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curious case of what are known as double hot

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Jupiters. These are rare exoplanet pairs

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found in binary star systems, with one

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scorching gas giant orbiting each of the twin

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stars. This arrangement has long puzzled

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scientists, seeming to defy our understanding

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of how planets form. But now a team

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of astronomers believes they have the key to

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this celestial puzzle, a process known as von

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Zypolidov Kozai or zlk. Migration

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team leader and Yale University astronomer

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Melena Rice describes it as a dance of sorts

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of essentially in a binary star system,

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the gravitational influence of the second

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star can significantly shape and warp the

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orbits of planets, causing them to migrate

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inward towards their parent stars. The

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researchers propose that this mechanism leads

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to a mirrored migration process, resulting in

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both stars in the binary system ending up

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with their own hot Jupiter. To reach this

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conclusion, Rice and her colleagues performed

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numerous simulations of binary stars with two

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planets using powerful computing clusters and

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data from sources like NASA's Exoplanet

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Archive and the European Space Agency's Gaia

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mission. The unintended yet

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exciting consequence of this research is that

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it makes our planet formation models a whole

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lot more interesting. We typically expect

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giant planets to form much further away from

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their host stars. Which is precisely why Hot

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Jupiters, especially pairs of them, have been

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such a captivating subject of studying. For

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future discoveries, the team suggests

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revisiting binary systems where just one Hot

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Jupiter has already been found. The crucial

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factor, however, is that these parent stars

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need to have a moderate separation, not too

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close and not too far apart, just the right

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distance for this gravitational dance to

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unfold.

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Next up, the global launch manifest continues

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to be as busy as ever. As we approach the

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halfway point of 2025 this week,

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we're looking at a packed schedule

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highlighted by multiple SpaceX Falcon 9

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missions, including a significant private

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crewed flight to the International Space

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Station. First up, Axiom Space aims to return

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crew to the iss with its fourth private

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mission, AX4, launching today if all goes

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according to plan. From Florida Commanding

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this flight is Peggy Whitson, a former NASA

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astronaut, making this her second commercial

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mission and further extending her record for

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the longest cumulative time in space by an

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American. Joining her are Shubanshu

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Shukla from India and mission specialists

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Slawash Usnanski, Wisniewski of Poland and

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Tibor Kapu of Hungary, all making their first

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space flights and marking significant

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milestones for their nations. This mission

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also debuts crew Dragon

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C213, the final capsule ever

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manufactured completing SpaceX's fleet. The

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Falcon 9 booster will attempt a, uh, return

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to launch site landing. Beyond the

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crewed mission, SpaceX is maintaining its

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impressive pace with three Starlink satellite

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deployments also on the docket. This week,

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two Falcon 9 flights will launch from Cape

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Canaveral carrying Starlink V2 mini

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satellites into low Earth orbit, while the

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third lifts off from Vandenberg Space Force

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Base in California. These launches underscore

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SpaceX's aggressive goal of completing 170

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orbital flights this year. Elsewhere on the

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launch pad, Rocket Lab aims to continue its

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record cadence with the 67th electron

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mission, symphony in the Stars from New

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Zealand. Slightly delayed for checkouts,

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this confidential commercial payload is set

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for a 650 kilometer orbit.

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Blue Origin also has its fifth New Shepard

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suborbital flight of 2025

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NS33, expected to carry a crew of

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six passengers, just above the Carmen line

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for a brief period of microgravity after

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being scrubbed last weekend. And

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finally, a momentous launch marks the end of

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an era, the 50th and final mission for

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the Japanese H2A rocket. This

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swan song flight, delayed due to an

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electrical issue, will carry the GOSAT GEO

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Water Earth Observation payload from the

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Tanegashima Space Center. This satellite is

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designed to monitor greenhouse gases and

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measure water on Earth's surface and in the

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atmosphere. The H2A, with an

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impressive track record, is being phased out

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in favor of its successor, the H3 family.

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And with that news, we wrap up today's

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episode of Astronomy Daily, where we explored

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everything from lunar lander challenges and a

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European spacecraft's re entry setback to the

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clumpy nature of our Milky Way and the hidden

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asteroids of Venus. Plus the fascinating

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dance of double hot Jupiters and a look at

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the busy week ahead for space launches. Thank

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you for joining us. I'm Anna your your host

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and I hope you enjoyed this dive into the

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cosmos. Remember, you can visit

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Astronomy Daily IO to catch up on all the

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latest space and astronomy news with our

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constantly updating newsfeed and listen to

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all our back episodes. Subscribe to Astronomy

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Daily on Apple Podcasts, Spotify,

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YouTube Music or wherever you get your

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podcasts. We'll see you again tomorrow. In

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the meantime, keep looking up

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stories be told

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stories.
