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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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China’s Tianwen-2 Set for Launch to Asteroid and Comet

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China’s Tianwen-2 Set for Launch to Asteroid and Comet

China has taken a major step forward in its deep-space exploration efforts as the Tianwen-2 spacecraft arrived at the Xichang Satellite Launch Center in Sichuan province for final launch preparations. The China National Space Administration (CNSA) confirmed the development on February 20, 2025, signaling that the mission is on track for its scheduled launch in the first half of the year.

A Dual-Purpose Mission

The Tianwen-2 mission is a combined near-Earth asteroid sample return and comet rendezvous mission, marking another ambitious endeavor for China’s space program. The mission is set to launch aboard a Long March 3B rocket, with a tentative liftoff expected around May 2025.

The primary target of Tianwen-2 is the near-Earth asteroid Kamoʻoalewa (2016 HO3), a small celestial body with a diameter estimated between 40 to 100 meters. The asteroid is considered a quasi-satellite of Earth, meaning it follows a co-orbital path with our planet. Scientists believe Kamoʻoalewa might be a fragment of the Moon, ejected into space after an ancient impact event.

After collecting samples from Kamoʻoalewa, the main spacecraft will continue its journey to comet 311P/PANSTARRS, a celestial body that exhibits both asteroid-like and comet-like characteristics. By studying these two objects, scientists aim to gain valuable insights into the composition, evolution, and history of the solar system, including the distribution of water and organic molecules.

Launch Preparations Underway

CNSA stated that the launch site facilities are fully prepared, and pre-launch tests are proceeding as planned. Engineers and scientists are meticulously working to ensure the spacecraft is ready for its complex mission, which will involve multiple orbital maneuvers, sample collection, and deep-space travel over nearly a decade.

Sampling Kamoʻoalewa: Two Innovative Techniques

To collect material from Kamoʻoalewa, Tianwen-2 will employ two advanced sampling methods:

  1. Touch-and-Go (TAG) Method – This technique, used by NASA’s OSIRIS-REx and JAXA’s Hayabusa2 missions, involves briefly touching the asteroid’s surface to gather samples.
  2. Anchor-and-Attach System – This approach uses drills attached to the spacecraft’s landing legs, allowing for a more stable and secure extraction of subsurface material.

Early mission concepts, when Tianwen-2 was initially known as Zheng He, indicated that China aimed to collect between 200 and 1,000 grams of asteroid samples. These samples will help scientists analyze Kamoʻoalewa’s mineral composition, origin, and potential similarities with lunar material.

Challenges in Sample Return

Although China has successfully executed two lunar sample return missions—Chang’e-5 (2020) and Chang’e-6 (2024)—returning asteroid samples presents unique challenges. Unlike the Moon, Kamoʻoalewa has negligible gravity, requiring specialized landing and sampling techniques. Additionally, the reentry module carrying the samples will experience higher velocities, demanding advanced thermal protection and parachute deployment systems.

To address these challenges, the China Aerospace Science and Technology Corporation (CASC) conducted high-altitude parachute tests in 2023, ensuring the safe return of asteroid samples to Earth around 2027.

Comet Rendezvous: Studying 311P/PANSTARRS

Returning samples from Kamoʻoalewa will not mark the end of Tianwen-2’s mission. The spacecraft will execute a gravitational slingshot maneuver around Earth, propelling it toward comet 311P/PANSTARRS in the main asteroid belt. The rendezvous is expected around 2034.

311P/PANSTARRS is considered a transitional object between asteroids and comets, making it an ideal candidate for studying the origins of cometary activity within the asteroid belt. Scientists hope to analyze its orbit, rotation, surface composition, volatile elements, and dust emissions, shedding light on the evolution of comets in the inner solar system.

Scientific Instruments on Board

The Tianwen-2 spacecraft is equipped with a suite of cutting-edge instruments to study its targets, including:

  • Multispectral and infrared spectrometers – To analyze surface composition.
  • High-resolution cameras – To map geological features in detail.
  • Radar sounder – To probe subsurface structures.
  • Magnetometer – To search for residual magnetic fields.
  • Dust and gas analyzers – To examine cometary activity.
  • Charged particle detectors – To study interactions with the solar wind (developed in collaboration with the Russian Academy of Sciences).

China’s Expanding Deep-Space Ambitions

Tianwen-2 follows the highly successful Tianwen-1 Mars mission, which saw China land the Zhurong rover on Mars in 2021. The Tianwen series is a key part of China’s growing presence in deep-space exploration:

  • Tianwen-3 – A Mars sample return mission, scheduled for 2028–2030.
  • Tianwen-4 – A Jupiter system exploration mission, launching around 2030, featuring a solar-powered orbiter for Callisto and a radioisotope-powered spacecraft for a Uranus flyby.

Chinese researchers have emphasized the importance of asteroid sample return missions, citing their potential for groundbreaking scientific discoveries and the development of new space technologies.

With Tianwen-2, China is taking a bold step into the future of deep-space exploration. By returning samples from an asteroid and studying a comet, the mission will provide crucial insights into the origins of the solar system and planetary evolution. As launch preparations continue, the world eagerly anticipates another milestone in China’s space program.

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SpaceX to Launch 21 Starlink Satellites from Florida on February 4

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SpaceX to Launch 21 Starlink Satellites from Florida on February 4

SpaceX plans to launch another batch of Starlink satellites into orbit from Florida’s Space Coast on February 4, 2025. The mission will deploy 21 Starlink satellites, including 13 equipped with direct-to-cell communications capabilities, marking another major step in SpaceX’s ambitious plan to provide global high-speed internet coverage.

The Falcon 9 rocket flight from Cape Canaveral Space Force Station is scheduled to take place during a roughly three-hour launch window that opens at 3:37 a.m. (0837 GMT). SpaceX will livestream the event on its X account (formerly Twitter), with coverage beginning about five minutes before liftoff.

The mission will use the experienced Falcon 9 first-stage rocket, which will be making its 21st launch and landing. According to SpaceX, this rocket has already flown on 20 missions, 16 of which were dedicated Starlink launches. If all goes as planned, the rocket will return to Earth about eight minutes after liftoff, landing on the unmanned “Just Read the Instructions” craft in the Atlantic Ocean.

The Falcon 9 upper stage will continue its journey to deploy 21 Starlink satellites into low Earth orbit (LEO) about 65 minutes after liftoff. This will be SpaceX’s 15th Falcon 9 mission in 2025, with nine flights dedicated to expanding the Starlink constellation.

Direct-to-cell capabilities


A notable feature of this mission is the inclusion of 13 Starlink satellites with direct-to-cell capability. These advanced satellites are designed to enable seamless connectivity for standard mobile phones, eliminating the need for specialized hardware. This technology has the potential to revolutionize communications in remote and underserved areas, providing reliable internet and cellular services directly to users’ devices.

The growing Starlink constellation


SpaceX is rapidly expanding its Starlink network, which is already the largest satellite constellation ever assembled. In 2024 alone, the company launched more than 130 Falcon 9 missions, about two-thirds of which were dedicated to Starlink deployments. According to astrophysicist and satellite tracker Jonathan McDowell, SpaceX currently operates nearly 7,000 Starlink satellites in LEO.

The Starlink network aims to provide high-speed, low-latency internet access to users around the world, especially in regions lacking traditional infrastructure. With this latest launch, SpaceX is expanding the network’s capacity and coverage, bringing its dream of global connectivity closer to reality.

Recyclability and sustainability


The Falcon 9 rocket’s first-stage booster exemplifies SpaceX’s commitment to reusability, a key factor in reducing the cost of spaceflight. By successfully landing and reusing the rocket, SpaceX has revolutionized the aerospace industry and set a new standard for sustainable space operations.

However, the rapid expansion of the Starlink constellation has raised concerns among astronomers and environmentalists. The growing number of satellites in LEO has created problems such as light pollution, which can interfere with astronomical observations, and space debris, which poses a threat to other spacecraft. SpaceX is actively working to mitigate these issues by implementing measures such as blacking out satellite surfaces and responsibly deorbiting inactive satellites.

The February 4 launch is part of SpaceX’s broader strategy to achieve global internet coverage and support its growing customer base. With the addition of direct-to-cell-connect satellites, the company is poised to offer even more versatile and simple connectivity solutions.

As SpaceX pushes the boundaries of space technology, the world will be watching to see how the Starlink network evolves and addresses the challenges associated with large-scale satellite constellations. For now, the focus is on the upcoming launch, which will mark another milestone in SpaceX’s journey to connect the world.

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Scientists Trap Molecules for Quantum Tasks, Paving the Way for Ultra-Fast Tech Advancements

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Scientists Trap Molecules for Quantum Tasks, Paving the Way for Ultra-Fast Tech Advancements

In a groundbreaking milestone for quantum computing, researchers from Harvard University have successfully trapped molecules to perform quantum operations. This achievement marks a pivotal advancement in the field, potentially revolutionizing technology and enabling ultra-fast computations in medicine, science, and finance.

Molecules as Qubits: A New Frontier

Traditionally, quantum computing has focused on using smaller, less complex particles like ions and atoms as qubits—the fundamental units of quantum information. Molecules, despite their potential, were long considered unsuitable due to their intricate and delicate structures, which made them challenging to manipulate reliably.

However, the latest findings, published in the journal Nature, change this narrative. By utilizing ultra-cold polar molecules as qubits, the researchers have opened up new possibilities for performing quantum tasks with unprecedented precision.

A 20-Year Journey to Success

“This is a breakthrough we’ve been working toward for two decades,” said Kang-Kuen Ni, Theodore William Richards Professor of Chemistry and Physics at Harvard and senior co-author of the study.

Quantum computing leverages the principles of quantum mechanics to perform calculations exponentially faster than classical computers. It has the potential to solve problems that were once deemed unsolvable.

“Our work represents the last critical piece needed to construct a molecular quantum computer,” added co-author and postdoctoral fellow Annie Park, highlighting the significance of this achievement.

How Molecular Quantum Gates Work

Quantum gates, the building blocks of quantum operations, manipulate qubits by taking advantage of quantum phenomena like superposition and entanglement. Unlike classical logic gates that process binary bits (0s and 1s), quantum gates can process multiple states simultaneously, exponentially increasing computational power.

In this experiment, the researchers used the ISWAP gate, a crucial component that swaps the states of two qubits while applying a phase shift. This process is essential for creating entangled states—a cornerstone of quantum computing that allows qubits to remain correlated regardless of distance.

Overcoming Long-Standing Challenges

Earlier attempts to use molecules for quantum computing faced significant challenges. Molecules were often unstable, moving unpredictably and disrupting the coherence required for precise operations.

The Harvard team overcame these obstacles by trapping molecules in ultra-cold environments. By drastically reducing molecular motion, they achieved greater control over quantum states, paving the way for reliable quantum operations.

The breakthrough was a collaborative effort between Harvard researchers and physicists from the University of Colorado’s Center for Theory of Quantum Matter. The team meticulously measured two-qubit Bell states and minimized errors caused by residual motion, laying the groundwork for even more accurate future experiments.

Transforming the Quantum Landscape

“There’s immense potential in leveraging molecular platforms for quantum computing,” Ni noted. The team’s success is expected to inspire further innovations and ideas for utilizing the unique properties of molecules in quantum systems.

This advancement could significantly alter the quantum computing landscape, bringing researchers closer to developing a molecular quantum computer. Such a system would harness the unique capabilities of molecules, opening doors to unprecedented computational possibilities.

The Road Ahead

The implications of this achievement extend far beyond academia. By unlocking the potential of molecules as qubits, the researchers have taken a vital step toward creating powerful quantum computers capable of transforming industries ranging from pharmaceuticals to financial modeling.

As researchers continue to refine this technology, the dream of a molecular quantum computer—one that capitalizes on the complexities of molecular structures—moves closer to reality. This breakthrough represents not just a leap forward for quantum computing but a glimpse into the future of technology itself.

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