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Weird science facts

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Usually, with science homework help you learn some essential facts about life like about forces that work in our world or molecular structure. But it is often very formal and not exciting. What about fun facts that will make science more interesting?

1. Babies have more bones than adults

At birth, babies have approximately 300 bones and cartilage between them. This flexibility allows them to pass through the birth canal, and also allows them to grow quickly. Many bones fuse with age. There are 206 bones in an average adult skeleton.

2. During the summer, the Eiffel Tower can reach 15 cm higher

Thermal expansion is the movement of particles in a substance when it is heated up. This is what is called a thermal expansion. A drop in temperature can cause it to contract. For example, the mercury level in a thermometer will rise and fall as the mercury volume changes with the temperature. This effect is strongest in gases, but it also occurs in liquids and solids like iron. This is why large structures like bridges have expansion joints that allow them to expand and contract without causing damage.

3. The Amazon rainforest produces 20% of Earth’s oxygen

The atmosphere is composed of approximately 78% nitrogen and 21% oxygen. There are also small amounts of other gases. Most living organisms on Earth require oxygen for survival. They convert it into carbon dioxide when they breathe. Photosynthesis is a way for plants to replenish oxygen levels on the planet. This process converts carbon dioxide and water into energy and releases oxygen as a byproduct. The Amazon rainforest covers 5.5 million km2 (2.1 million sq miles). It absorbs large amounts of carbon dioxide and cycles significant quantities of oxygen.

4. Some metals explode when they come in contact with water

Certain metals, such as potassium, sodium and rubidium, oxidize (or tarnish) quickly when exposed to oxygen. Dropping them in water can cause explosions. Chemical stability is a goal for all elements. This means that they must have an outer electron shell. Metals are known to lose electrons in order to achieve this. Alkali metals only have one electron in their outer shell, which makes them extremely eager to pass this unwelcome passenger on to another element through bonding. They form compounds with other elements so easily that they can’t exist in their own right.

5. 6 billion tonnes for a teaspoonful of neutron stars

A neutron star is a remnant of a large star that has run out of fuel. A supernova occurs when a dying star explodes, and its core collapses under gravity to form a super-dense neutron star. The staggeringly large solar masses of galaxies or stars are measured by astronomers in solar masses. This is equivalent to 2 x 1030 kg/4.4 x 1030 lbs. The typical neutron star has a mass up to three solar masses. This is compressed into a sphere of approximately ten kilometers (6.2 miles), which results in some of the most dense matter in the universe.

6. Every year, Hawaii moves 7.5 cm closer to Alaska

The Earth’s crust has been split into huge pieces known as tectonic plates. These plates move in constant motion due to currents in Earth’s upper crust. Hotter, denser rock rises and then cools and sinks. This creates circular convection currents that act as giant conveyor belts that slowly shift the tectonic plates. Hawaii is located in the middle Pacific Plate. It slowly drifts north-west towards the North American Plate and back to Alaska. The speed of the plates is similar to how fast our fingernails grow.

7. Chalk is made of trillions upon trillions of microscopic plankton fossils

Coccolithophores are tiny single-celled algae that have been living in the oceans of Earth for over 200 million years. They surround themselves with tiny plates of calcite (coccoliths), which is unlike any other marine plant. Coccolithophores formed in thick layers on ocean floors, covering them with a white ooze. This was just 100 million years ago. The pressure from the ocean floor pushed the coccoliths into rock. This created chalk deposits like the Dover white cliffs. Coccolithophores is just one example of many prehistoric species that are preserved in fossil form. But how can we determine how old they really are? Rock forms in horizontal layers over time. Older rocks are at the bottom, while younger rocks are near the top. Paleontologists can approximate the age of a fossil by studying the rock from which it is found. Based on radioactive elements like carbon-14, carbon dating gives a more precise estimate of a fossil’s age.

8. It will be too hot to sustain life on Earth in 2.3 billion years

The Sun will get brighter and more intense over the next hundreds of millions of year. Temperatures will rise to the point that our oceans will evaporate in just 2 billion years. This will make it impossible for Earthlings to live. Our planet will soon become a desert like Mars. Scientists predict that Earth will eventually be engulfed by the Sun as it grows into a red giant over the next few billion years.

9. Infrared cameras are almost impossible to detect polar bears

The heat that is lost by a subject can be detected using thermal cameras, but polar bears have mastered the art of conserving heat. A thick layer of blubber beneath the skin keeps bears warm. They can withstand even the coldest Arctic days thanks to their dense fur coat.

10. It takes light 8 minutes and 19 seconds to travel from Earth to Sun

Light travels 300,000 km (186,000 miles per second) in space. It takes a lot of time to cover the 150 million kilometres (93,000,000 miles) between us, the Sun, and this speed. Eight minutes is still a lot compared to the five-and-a-half hours required for the Sun’s light to reach Pluto.

11. The human race could be reduced to the size of a sugar cube if all the space in our atoms was removed

Although the atoms that make up our world appear solid, they are actually 99.99999 percent empty space. An atom is composed of a small, dense nucleus, surrounded by electrons and spread over a large area. Because electrons behave like waves, they are particles as well. The crests and the troughs of these waves are what make electrons exist. Instead of being located in a single point, electrons are distributed over multiple probabilities. This is called an orbital. These electrons occupy huge amounts of space.

12. Stomach acid can dissolve stainless steel

The highly corrosive acid hydrochloric acid, which has a pH between 2 and 3, affects the digestion of food. Your stomach lining is also affected by this acid. It secretes an alkali bicarbonate solution to protect itself. It is necessary to replace the lining every day, and it completely renews itself every four.

13. The Earth is a huge magnet

The Earth’s inner core is made up of a sphere filled with solid iron and surrounded by liquid iron. Temperature and density variations create currents in the iron that in turn produces electrical currents. These currents, paired up by the Earth’s rotation, create a magnetic field that is used worldwide by compass needles.

14. Venus is the only planet that can spin clockwise

Our Solar System began as a swirling cloud made of gas and dust. It eventually became a spinning disc with our Sun at its centre. All the planets orbit the Sun in roughly the same direction because of this common origin. They all also spin in the same direction (counterclockwise, if observed from above), except Uranus & Venus. Uranus spins on its back, while Venus spins in the opposite direction. These planetary anomalies are most likely caused by gigantic asteroids that have thrown them off track in the distant past.

15. A flea can accelerate quicker than the Space Shuttle

Jumping fleas can reach heights of eight centimetres (three in) in one millisecond. Acceleration refers to the change in speed over time. It is often measured in ‘gs. One g equals the acceleration caused on Earth by gravity (9.8m/32.2ft per square second). Fleas can experience 100g while the Space Shuttle was able to reach around 5g. This is due to a rubber-like protein that allows it to store and release energy just like a spring.

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A NASA spacecraft ‘touches the sun’ during a turning point in human history

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On Christmas Eve, NASA’s Parker Solar Probe set a new record by approaching the sun’s surface within barely 3.86 million miles (6.1 million kilometers). Parker’s historic moment can be followed on NASA’s Eyes On The Solar System page.

On Tuesday, December 24, a fully armored NASA spacecraft, barely larger than a tiny car, became the closest man-made object to the sun in history, marking one of humanity’s most amazing space exploration achievements. In addition, the fastest item ever created by humans broke its speed record, and humanity made its closest visit to a star ever.

A Monumental Performance

At 11:53 UTC (6:53 a.m. EST) on Tuesday, December 24, Parker accomplished an unprecedented close flyby of the sun, coming within barely 3.86 million miles (6.1 million kilometers) of its surface. This was a tremendous accomplishment of exploration. It had come this near to the sun 22 times.

It is the closest man-made object to the sun ever, at 96% of the distance between the sun and Earth, well within Mercury’s orbit at roughly 39%.

The project’s scientist at the Johns Hopkins Applied Physics Laboratory, Dr. Nour Raouafi, compares the importance of this mission to the 1969 moon landing. During a media roundtable at the annual conference of the American Geophysical Union on December 10, 2024, he declared, “It’s the moment we have been waiting for for nearly 60 years.” “In 1969, we landed humans on the moon. On Christmas Eve, we embrace a star — our star.”

‘Hyper-Close’

Parker will slice through plasma plumes that are still attached to the sun in what NASA refers to as a “hyper-close regime,” getting close enough to pass inside a solar outburst “like a surfer diving under a crashing ocean wave.”

According to Raouafi, the heat Parker will experience when it is closest to the sun is “nearly 500 times the hottest summer day we can witness on Earth.”

Parker was already the fastest thing ever constructed on Earth, but it will surpass all previous records for speed and distance when it approaches the sun at 430,000 mph (690,000 kph). The mission’s website states that it would take one second to go from Philadelphia to Washington, D.C.

On December 27, 2024, mission operators at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, will wait for a beacon tone to certify the probe’s survival after losing touch with it for three days.

On March 22 and June 19, 2025, Parker will make two additional hyper-close passes at the same distance.

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Researchers Achieve Breakthrough in Quantum Simulation of Electron Transfer

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A team at Rice University has achieved a significant breakthrough in simulating molecular electron transfer using a trapped-ion quantum simulator. Their research offers fresh insights into the dynamics of electron transfer and could pave the way for innovations in molecular electronics, renewable energy, and cc.

Electron transfer is a critical process underpinning numerous physical, chemical, and biological phenomena. However, the complexity of quantum interactions has long made it a challenging area to study. Conventional computational techniques often struggle to capture the full range of variables influencing electron transfer.

To address these challenges, the researchers developed a programmable quantum system capable of independently controlling key factors such as donor-acceptor energy gaps, electronic and vibronic couplings, and environmental dissipation. Using ions trapped in an ultra-high vacuum and manipulated by laser light, the team demonstrated real-time spin dynamics and measured electron transfer rates.

“This is the first time that this kind of model has been simulated on a physical device while incorporating the role of the environment and tailoring it in a controlled way,” said Guido Pagano, lead author of the study published in Science Advances.

Pagano added, “It represents a significant leap forward in our ability to use quantum simulators to investigate models and regimes relevant to chemistry and biology. By harnessing the power of quantum simulation, we hope to explore scenarios currently inaccessible to classical computational methods.”

Through precise engineering of tunable dissipation and programmable quantum systems, the researchers explored both adiabatic and nonadiabatic regimes of electron transfer. The experiment not only illuminated how quantum effects function under diverse conditions but also identified optimal parameters for electron transfer.

The team emphasized that their findings bridge a critical gap between theoretical predictions and experimental verification. By offering a tunable framework to investigate quantum processes in complex systems, their work could lead to groundbreaking advancements in renewable energy technologies, molecular electronics, and the development of novel materials.

“This experiment is a promising first step toward understanding how quantum effects influence energy transport, particularly in biological systems like photosynthetic complexes,” said Jose N. Onuchic, study co-author. “The insights gained could inspire the design of more efficient light-harvesting materials.”

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Crew Dragon Mission Delay Extends Astronauts’ Stay on ISS by a Month

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The next mission of SpaceX’s Crew Dragon to the International Space Station (ISS) has been postponed by a month due to delays in completing a new spacecraft. This decision will extend the stay of some astronauts aboard the ISS, including two who have been there since June.

NASA announced on December 17 that the Crew-10 mission, initially scheduled for February, is now set to launch no earlier than late March. The delay stems from the need for additional time to finish the fabrication, assembly, testing, and integration of a new Crew Dragon capsule.

Crafting the New Dragon Capsule

“Fabrication, assembly, testing, and final integration of a new spacecraft is a painstaking endeavor that requires great attention to detail,” said Steve Stich, NASA’s Commercial Crew Program Manager. He commended SpaceX’s efforts to expand the Dragon fleet and the flexibility of the ISS crew in accommodating the delay.

The new Crew Dragon will be the fifth in SpaceX’s lineup of crewed spacecraft, complementing its three cargo Dragon vehicles. According to Sarah Walker, SpaceX’s Dragon Mission Management Director, the spacecraft was near completion as of July and was undergoing final work at SpaceX’s California facility. It is now expected to arrive in Florida for final preparations in January.

While NASA did not specify the exact reasons for the delay, it considered other options, including using an existing Crew Dragon or making adjustments to the launch manifest, before opting for the delay. Existing capsules, including Freedom, currently at the ISS, and Endeavour and Resilience, which recently returned from other missions, were not available for a February launch.

Crew Adjustments and Extended ISS Stay

The Crew-10 mission will proceed with its planned roster: Anne McClain and Nichole Ayers from NASA, Takuya Onishi from JAXA, and Kirill Peskov from Roscosmos.

The delay has implications for the Crew-9 mission, launched in late September with NASA astronaut Nick Hague and Roscosmos cosmonaut Aleksandr Gorbunov. They were joined by NASA astronauts Suni Williams and Butch Wilmore, who have been on the station since June after arriving on Boeing’s CST-100 Starliner.

Originally, Williams and Wilmore were scheduled to stay for just over a week, but their time on the ISS will now extend to about 10 months. NASA had earlier decided to return the uncrewed Starliner to Earth due to concerns with its thrusters.

Despite the delay, NASA emphasizes that Williams and Wilmore are not “stranded” as they can return to Earth in an emergency. Their extended stay is tied to the decision to use the new Crew Dragon for the upcoming mission, as preparing another vehicle was deemed impractical.

Looking Ahead

Assuming the Crew-10 launch proceeds in late March, the Crew-9 spacecraft is expected to return to Earth in early April after a handover period. This delay underscores the complexity of preparing new spacecraft while ensuring the safety and readiness of all missions.

As the new Crew Dragon nears completion, SpaceX and NASA remain focused on maintaining seamless operations aboard the ISS and advancing human space exploration.

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