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SpaceX is slated to launch its gargantuan Starship rocket on Tuesday out of South Texas, a key test that is expected to include a guest visit from President-elect Donald Trump.

The sixth major test mission comes as SpaceX Chief Executive Officer Elon Musk is heavily engaged in transition planning for Trump’s second administration. Musk, who has been a near-constant fixture of Trump’s inner circle since the November 5 election, has maintained that over regulation, especially surrounding Starship, factored into his decision to support the Republican.

SpaceX will try to launch Starship from its site in South Texas during a 30-minute time slot beginning at 4 p.m. local time, sending the vehicle to space and partially around the world.

One of the most anticipated moments on Tuesday will come about seven minutes into the mission when the company will attempt to catch the Super Heavy booster in midair with giant mechanical arms — referred to as “chopsticks” — repeating the groundbreaking feat from its previous flight.

The largest and most powerful rocket ever developed, Starship is under contract to function as a lunar lander that NASA will use to put people back on the moon for the first time in half a century. It’s the centerpiece of Musk’s ambition to start a settlement on Mars. 

The vehicle is also meant to revolutionise SpaceX’s business plan. Designed to be fully reusable, SpaceX claims Starship will be much cheaper to fly than any other rocket on the market and will eventually replace its industry-leading Falcon 9 and Falcon Heavy rockets for sending cargo into orbit. 

But to meet that promise of delivering a fully reusable rocket, SpaceX must refine its technique for recovering all of the pieces of Starship after launch. 

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The launch will be the latest event Musk and Trump have attended together, following a Saturday night Ultimate Fighting Championship match in Madison Square Garden. Trump has frequently showered Musk with praise at his rallies, oftentimes describing in great detail his awe watching SpaceX rockets. 

On this flight, the company will attempt once again to “catch” the rocket’s massive booster, called Super Heavy, which is used to propel the Starship spacecraft toward space throughout the first few minutes of takeoff. Like last time, the booster will return back its launchpad and slow itself down as it comes in for landing. A pair of giant mechanical arms will then catch the booster and stop its fall.

Starship will attempt a fiery return plunge through the atmosphere, testing out an updated heat shield to protect it during the fall. It will then try to return to an upright position before splashing down into the Indian Ocean.

While most of Starship appeared to survive this process in October, parts of the vehicle appeared to burn off. However, the company was still able to splash down Starship relatively intact and upright in the ocean.

SpaceX should have a better view of this fall during Tuesday’s launch attempt. The company aims to launch in the Texas afternoon, which means Starship will be landing in the Indian Ocean during the daytime. That should provide more sunlight to show how the vehicle survives its descent.

SpaceX President Gwynne Shotwell said on Friday that as many as 400 Starship flights were possible over the next four years. That frequency can only happen if SpaceX perfects its landing strategy, so the company can quickly turn around the rockets for their next flights. Shotwell described the process as similar to the way airlines drive down the cost of owning and operating commercial jetliners.

During the October test, the booster came very close to crashing near the tower, Musk said in a video on his X platform. SpaceX will need to address that issue as well as a laundry list of other things, such as refueling the vehicle in space, before Starship lives up to the full scope of Musk’s plans.

© 2024 Bloomberg L.P.

(This story has not been edited by NDTV staff and is auto-generated from a syndicated feed.)

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Ancient 2,600-Year-Old Inscription in Turkey Finally Decoded

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Ancient 2,600-Year-Old Inscription in Turkey Finally Decoded

A 2,600-year-old inscription engraved on a monument in Turkey, known as Arslan Kaya or “lion rock,” has been deciphered, according to research by Professor Mark Munn of Pennsylvania State University. This ancient carving, which has endured significant damage from weathering and looting, contains references to Materan, a goddess revered by the Phrygians, an ancient civilisation that thrived in the region between 1200 and 600 B.C. Materan, often simply called “the Mother,” was central to Phrygian religious beliefs.

Monument Details and Historical Significance

The Arslan Kaya monument is decorated with images of lions and sphinxes, which were symbols of strength and protection in Phrygian culture. The name Materan, deciphered through careful analysis of the damaged inscription, appears alongside a depiction of the goddess. Materan was later venerated by other cultures, known as “Mother of the Gods” by the Greeks and as “Magna Mater” or “Great Mother” by the Romans.

At the time the inscription was created, the region was under the influence of the Lydian kingdom, which also held Materan in high regard. The inscription, believed to have been part of a longer text, may have detailed the commissioning party and explained the goddess’s significance.

Challenges in Deciphering the Inscription

The text has been the subject of scholarly debate for over a century. Munn utilised detailed photographs and historical records to piece together its meaning, noting that optimal lighting on April 25, 2024, played a crucial role in capturing the monument’s details.

Rostyslav Oreshko, a lecturer at the Practical School of Advanced Studies in France, told LiveScience that Munn’s work affirms earlier readings from the 19th century, which identified the name Materan. Despite this, Oreshko emphasised that the study solidifies previous interpretations rather than offering entirely new insights.

The deciphered inscription sheds light on the enduring cultural significance of Materan and highlights the Phrygians’ influence on subsequent civilisations.

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Dolphin in Baltic Sea Talks to Himself, Might Feel Alone Claims Scientists

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Dolphin in Baltic Sea Talks to Himself, Might Feel Alone Claims Scientists

A bottlenose dolphin residing alone in the Baltic Sea has been documented producing thousands of vocalisations, potentially as a result of loneliness. Known locally as Delle, this dolphin was first noticed in the Svendborgsund channel near Funen Island, Denmark, in 2019. Bottlenose dolphins typically thrive in social pods, but no other dolphins have been seen in the area.

The University of Southern Denmark deployed underwater recorders to monitor the impact of Delle’s presence on local harbour porpoises. Unexpectedly, 10,833 sounds were recorded over 69 days between December 8, 2022, and February 14, 2023. Dr Olga Filatova, cetacean biologist and lead researcher, reported hearing an extensive range of sounds, including whistles and tonal noises. These sounds are often associated with social interactions among dolphins, yet Delle was entirely alone.

Unpacking the Recordings

Among the captured vocalisations were 2,291 whistles and 2,288 burst-pulses—clicks often linked to aggression or excitement. Delle also produced three distinctive whistles resembling “signature whistles”, unique sounds used by dolphins as individual identifiers. These findings, detailed in the journal Bioacoustics on October 31, led researchers to initially speculate that multiple dolphins might be present. However, Delle’s solitary state ruled out such assumptions.

Possible Explanations for the Vocalisations

The sounds may indicate attempts to connect with others or might simply reflect involuntary expressions linked to emotions, similar to humans laughing while alone. Dr Filatova suggested it is unlikely that Delle was calling other dolphins, as his years in the area would have revealed the absence of companions.

The study highlights a gap in understanding solitary dolphins’ behaviour. Thea Taylor, Managing Director of the Sussex Dolphin Project, noted the potential for these findings to provide insights into dolphin emotions and behaviour, stressing that solitary individuals remain under-researched.
Delle’s case underscores the complexity of dolphin communication, with researchers aiming to uncover the motivations behind such vocal patterns in isolated circumstances.

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New Research Explains Zebra Pattern in Radio Waves from Crab Nebula

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New Research Explains Zebra Pattern in Radio Waves from Crab Nebula

A puzzling ‘zebra’ pattern in high-frequency radio waves emitted by the Crab Nebula’s pulsar might finally have an explanation, according to new research by Mikhail Medvedev, Professor of Physics and Astronomy at the University of Kansas. This unique pattern, characterized by unusual frequency-based band spacing, has intrigued astrophysicists since its discovery in 2007. Medvedev’s findings, recently published in Physical Review Letters, suggest that wave diffraction and interference occurring in the pulsar’s plasma-rich environment could be responsible.

High-Frequency Radio Pulses Create Zebra-Like Patterns

The Crab Nebula, a remnant of a supernova observed nearly a millennium ago, features a neutron star known as the Crab Pulsar at its core. This pulsar, approximately 12 miles in diameter, emits electromagnetic radiation in sweeping pulses similar to a lighthouse beam. The Crab Pulsar stands out due to its distinct zebra pattern—observed only within a specific pulse component and spanning frequencies between 5 and 30 gigahertz.

Medvedev’s model theorizes that the zebra pattern arises from the pulsar’s dense plasma environment. The plasma, made up of charged particles like electrons and positrons, interacts with the pulsar’s magnetic field, affecting radio waves in ways that resemble diffraction phenomena seen in light waves. As these waves propagate through areas of varying plasma density, they create a pattern of bright and dark fringes, which ultimately appear as the zebra pattern observed from Earth.

Implications for Plasma Density Measurement and Neutron Star Research

Medvedev’s work sheds light on the peculiarities of the Crab Pulsar and offers a method for measuring plasma density in the magnetospheres of neutron stars. The model uses wave optics to analyse fringe patterns and determine the plasma’s distribution and density. This is a breakthrough that could open new avenues for studying other young and energetic pulsars. This innovative method provides what Medvedev describes as a “tomography of the magnetosphere,” enabling a density map of charged particles around neutron stars.

Further observational data will be needed to validate Medvedev’s theory, especially as astrophysicists seek to apply his method to other young, energetic pulsars. His model, if confirmed, could help to enhance our understanding of neutron stars’ plasma environments and the interactions of electromagnetic waves with pulsar plasma.

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