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Based on the principles of physics, it is theoretically possible for a planet to have a donut-shaped structure. To maintain the stability of a donut-shaped Earth, it would need to rotate at extremely high speeds, resulting in shorter day durations. Consequently, the gravitational force at the poles would intensify,... approximately twice as strong as at the equator. The Moon would continue to orbit the Earth, as long as it maintains a sufficient distance. If the donut-shaped Earth has no tilt, the inner edges would receive no sunlight, while the outer edges would experience increased sunlight exposure, leading to significant temperature variations and extreme weather conditions. However, if the tilt remains unchanged, both the inner and outer edges would receive adequate sunlight. It is worth noting that a naturally occurring donut-shaped planet is highly unlikely unless advanced extraterrestrial beings decide to create one.show more

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On January 14, 2005, the Huygens probe descending through Titan’s atmosphere revealed one of the rarest views in space exploration. From Saturn’s moon Titan, Earth and the Moon crossed in front of the Sun as tiny shadows nearly a billion miles away. What makes it even more incredible is how rare the alignment was. A perfectly central Earth and Moon transit from Saturn’s system happens only about twice every 1,000 years. From that distance, our entire planet looked small enough to disappear into the sunlight.

On January 14, 2005, the Huygens probe descending through Titan’s atmosphere revealed one of the rarest views in space exploration. From Saturn’s moon Titan, Earth and the Moon crossed in front of the Sun as tiny shadows nearly a billion miles away. What makes it even more incredible is how rare the alignment was. A perfectly central Earth and Moon transit from Saturn’s system happens only about twice every 1,000 years. From that distance, our entire planet looked small enough to disappear into the sunlight.

Cosmos Archive

35,727 Aufrufe • vor 2 Monaten

Kudos to Kevin Kisner getting the REAL issue when it comes to the modern golf ball… While discussing the ball Ray Floyd used to win the 1986 U.S. Open at Shinnecock, he correctly references SPIN more than SPEED. Yes, the modern ball flys WAY farther, but the easiest fix would be to mandate more spin on the ball. The worst part of the ball traveling insane distances is that, because of no real spin, the mishits do not go off line NEARLY as much as they used to. If the spin returned, hitting a 350 yard drive would carry with it the HUGE risk of a mishit heading for deep trouble, even bringing many out of bounds back into play. As a result, not only would hitting a driver create far more drama than it currently does, it would cause most players to self regulate by hitting 3-woods and irons off the tee to keep the ball in play. This would effectively solve the distance problem because it would cause significantly longer shots to be played into the greens. Please, USGA PGA of America PGA of AmericaTOUR The Masters The R&A THIS is the path!

Kudos to Kevin Kisner getting the REAL issue when it comes to the modern golf ball… While discussing the ball Ray Floyd used to win the 1986 U.S. Open at Shinnecock, he correctly references SPIN more than SPEED. Yes, the modern ball flys WAY farther, but the easiest fix would be to mandate more spin on the ball. The worst part of the ball traveling insane distances is that, because of no real spin, the mishits do not go off line NEARLY as much as they used to. If the spin returned, hitting a 350 yard drive would carry with it the HUGE risk of a mishit heading for deep trouble, even bringing many out of bounds back into play. As a result, not only would hitting a driver create far more drama than it currently does, it would cause most players to self regulate by hitting 3-woods and irons off the tee to keep the ball in play. This would effectively solve the distance problem because it would cause significantly longer shots to be played into the greens. Please, USGA PGA of America PGA of AmericaTOUR The Masters The R&A THIS is the path!

John Ziegler

549,754 Aufrufe • vor 1 Monat

If the British had gone to the moon and put up a flag it would probably have been classed as a hate crime 🤦‍♂️

If the British had gone to the moon and put up a flag it would probably have been classed as a hate crime 🤦‍♂️

Scott Cheggs

10,855 Aufrufe • vor 10 Monaten

When a spacecraft leaves Earth, it doesn’t just fire its engines and head straight to its destination. In many missions, especially those going beyond low Earth orbit, there’s a more subtle and elegant strategy at play, one that uses gravity itself as part of the navigation system. This is often called a gravity assist, or a slingshot maneuver. But in the case of missions like #Artemis II, what’s being used is a closely related idea known as a free-return trajectory. At first glance, it might sound simple: the spacecraft goes to the Moon, loops around it, and comes back. But the physics behind it is anything but simple. Instead of relying on continuous propulsion, the spacecraft follows a carefully calculated path through the gravitational field of the Earth–Moon system. It is launched with just the right speed and direction so that, as it approaches the Moon, the Moon’s gravity bends its trajectory. The spacecraft is effectively flung around the Moon, redirected onto a path that naturally brings it back toward Earth. No major engine burn is needed for the return. Small trajectory corrections may still be required, but gravity does the heavy lifting. That’s the key. This kind of trajectory is not just efficient, it’s also safe. If something goes wrong with the spacecraft’s engines or onboard systems, gravity itself ensures the return. It’s an inherent backup plan, built into the trajectory from the very beginning. The same fundamental idea appears in gravity assists used across the Solar System. When a spacecraft flies past a planet, it can gain or lose speed by exchanging momentum with that planet. From the spacecraft’s point of view, it’s as if it has been accelerated without using fuel. In reality, it has borrowed a tiny amount of orbital energy from the planet itself. That’s how missions like Voyager reached the outer planets, and how probes continue to explore regions far beyond what their onboard fuel alone would allow. But there’s an important distinction. An interplanetary gravity assist is typically used to change speed and direction, often increasing the spacecraft’s energy. A free-return trajectory, like the one used in Artemis II, is designed for something more specific: a path that naturally loops back to Earth without requiring additional propulsion. It’s less about gaining energy, and more about shaping a trajectory that guarantees a return. To understand why this works, it helps to stop thinking in straight lines. In space, motion follows curves defined by gravity. The spacecraft is constantly falling, first toward Earth, then toward the Moon, and then back toward Earth again. What looks like a loop is really a continuous free fall through a changing gravitational landscape. This way of navigating space reveals something deeper. We tend to think of engines as the drivers of motion, but once a spacecraft is on its way, gravity does most of the work. The art of spaceflight is not just about thrust. It’s about knowing when not to use it. #GoodLuck #Artemis NASA Artemis

When a spacecraft leaves Earth, it doesn’t just fire its engines and head straight to its destination. In many missions, especially those going beyond low Earth orbit, there’s a more subtle and elegant strategy at play, one that uses gravity itself as part of the navigation system. This is often called a gravity assist, or a slingshot maneuver. But in the case of missions like #Artemis II, what’s being used is a closely related idea known as a free-return trajectory. At first glance, it might sound simple: the spacecraft goes to the Moon, loops around it, and comes back. But the physics behind it is anything but simple. Instead of relying on continuous propulsion, the spacecraft follows a carefully calculated path through the gravitational field of the Earth–Moon system. It is launched with just the right speed and direction so that, as it approaches the Moon, the Moon’s gravity bends its trajectory. The spacecraft is effectively flung around the Moon, redirected onto a path that naturally brings it back toward Earth. No major engine burn is needed for the return. Small trajectory corrections may still be required, but gravity does the heavy lifting. That’s the key. This kind of trajectory is not just efficient, it’s also safe. If something goes wrong with the spacecraft’s engines or onboard systems, gravity itself ensures the return. It’s an inherent backup plan, built into the trajectory from the very beginning. The same fundamental idea appears in gravity assists used across the Solar System. When a spacecraft flies past a planet, it can gain or lose speed by exchanging momentum with that planet. From the spacecraft’s point of view, it’s as if it has been accelerated without using fuel. In reality, it has borrowed a tiny amount of orbital energy from the planet itself. That’s how missions like Voyager reached the outer planets, and how probes continue to explore regions far beyond what their onboard fuel alone would allow. But there’s an important distinction. An interplanetary gravity assist is typically used to change speed and direction, often increasing the spacecraft’s energy. A free-return trajectory, like the one used in Artemis II, is designed for something more specific: a path that naturally loops back to Earth without requiring additional propulsion. It’s less about gaining energy, and more about shaping a trajectory that guarantees a return. To understand why this works, it helps to stop thinking in straight lines. In space, motion follows curves defined by gravity. The spacecraft is constantly falling, first toward Earth, then toward the Moon, and then back toward Earth again. What looks like a loop is really a continuous free fall through a changing gravitational landscape. This way of navigating space reveals something deeper. We tend to think of engines as the drivers of motion, but once a spacecraft is on its way, gravity does most of the work. The art of spaceflight is not just about thrust. It’s about knowing when not to use it. #GoodLuck #Artemis NASA Artemis

Erika 

234,886 Aufrufe • vor 3 Monaten

This is one of the harshest industrial jobs on Earth. It pays $5,600 a week. Would you be able to do it?

This is one of the harshest industrial jobs on Earth. It pays $5,600 a week. Would you be able to do it?

Interesting AF

314,761 Aufrufe • vor 7 Monaten

ASTEROID 2024 YR4 MAY HIT THE MOON—AND SCIENTISTS ARE HOPING IT DOES A once-alarming asteroid is now offering a unique lunar science opportunity. Asteroid 2024 YR4, once feared to hit Earth, now poses no threat to our planet—but it might collide with the Moon. The 197-foot-wide space rock, tracked by the James Webb Space Telescope, now has a 2% chance of impacting the Moon, according to new data. Scientists say the impact would be harmless to Earth but groundbreaking for research. Julia de León, planetary scientist: "Honestly, I hope it does." If it strikes, it would mark the first time a 60-meter object has been observed slamming into the Moon live. Source: NASA Asteroid Watch

ASTEROID 2024 YR4 MAY HIT THE MOON—AND SCIENTISTS ARE HOPING IT DOES A once-alarming asteroid is now offering a unique lunar science opportunity. Asteroid 2024 YR4, once feared to hit Earth, now poses no threat to our planet—but it might collide with the Moon. The 197-foot-wide space rock, tracked by the James Webb Space Telescope, now has a 2% chance of impacting the Moon, according to new data. Scientists say the impact would be harmless to Earth but groundbreaking for research. Julia de León, planetary scientist: "Honestly, I hope it does." If it strikes, it would mark the first time a 60-meter object has been observed slamming into the Moon live. Source: NASA Asteroid Watch

Mario Nawfal

175,862 Aufrufe • vor 1 Jahr

The total lunar eclipse started at 23:28 on Sunday evening and conclude at 04:55 on Monday morning, Beijing time. The totality phase, known as the "red moon," will last from 01:31 to 02:53, with a duration of one hour and 22 minutes. "A lunar eclipse is rare. It occurs when the earth moves right in the middle of the moon and the sun, blocking the sunlight from shining on the moon. The total lunar eclipse this time will last for a relatively long time as it will enter the earth's shadow quite deeply. " said by an expert at Beijing Planetarium. This eclipse can be observed with the naked eye under good weather conditions.

The total lunar eclipse started at 23:28 on Sunday evening and conclude at 04:55 on Monday morning, Beijing time. The totality phase, known as the "red moon," will last from 01:31 to 02:53, with a duration of one hour and 22 minutes. "A lunar eclipse is rare. It occurs when the earth moves right in the middle of the moon and the sun, blocking the sunlight from shining on the moon. The total lunar eclipse this time will last for a relatively long time as it will enter the earth's shadow quite deeply. " said by an expert at Beijing Planetarium. This eclipse can be observed with the naked eye under good weather conditions.

KABClub

20,263 Aufrufe • vor 10 Monaten

On April 26th, 2026, the Japan Meteorological Agency's Himawari-8 satellite captured a full day of Earth. Every ten minutes, for twenty-four hours, it photographed a complete hemisphere of the planet. One hundred forty-four individual photographs. No editing for content. No compositing. No CGI. No green screen. No hologram. No drawings. These are photographs, assembled into video. Himawari-8 is a geostationary weather satellite operated by Japan. It orbits at roughly twenty-two thousand miles above the equator, remaining fixed over one spot on the planet, orbiting at the same rate Earth rotates. It was launched in 2014. It takes photographs of Earth in visible light and infrared. It does this every ten minutes, every single day, year after year. These images are available to the public. Meteorologists worldwide use them for weather forecasting. News organizations use them. Scientists use them. You can access them yourself right now. What you're seeing over that twenty-four hour period is the terminator line moving -- the day-night boundary shifting as the planet's rotation carries different regions into and out of sunlight, all viewed from a fixed point in space. It is not a composite. It is not a trick. The curvature you see is not distortion. It is not perspective compression. It is the actual shape of the Earth as photographed by an independent satellite operated by a nation with no interest in perpetuating a NASA conspiracy. This is what Earth looks like from space. This is the globe holding atmosphere in place with gravity as you witness weather patterns moving across its surface. This is reality. (No fisheye lens was harmed in the making of this video.)

On April 26th, 2026, the Japan Meteorological Agency's Himawari-8 satellite captured a full day of Earth. Every ten minutes, for twenty-four hours, it photographed a complete hemisphere of the planet. One hundred forty-four individual photographs. No editing for content. No compositing. No CGI. No green screen. No hologram. No drawings. These are photographs, assembled into video. Himawari-8 is a geostationary weather satellite operated by Japan. It orbits at roughly twenty-two thousand miles above the equator, remaining fixed over one spot on the planet, orbiting at the same rate Earth rotates. It was launched in 2014. It takes photographs of Earth in visible light and infrared. It does this every ten minutes, every single day, year after year. These images are available to the public. Meteorologists worldwide use them for weather forecasting. News organizations use them. Scientists use them. You can access them yourself right now. What you're seeing over that twenty-four hour period is the terminator line moving -- the day-night boundary shifting as the planet's rotation carries different regions into and out of sunlight, all viewed from a fixed point in space. It is not a composite. It is not a trick. The curvature you see is not distortion. It is not perspective compression. It is the actual shape of the Earth as photographed by an independent satellite operated by a nation with no interest in perpetuating a NASA conspiracy. This is what Earth looks like from space. This is the globe holding atmosphere in place with gravity as you witness weather patterns moving across its surface. This is reality. (No fisheye lens was harmed in the making of this video.)

Alex Boge

12,122 Aufrufe • vor 2 Monaten

Auroras danced across Alaska’s sky last night.😮🌌 A breathtaking sign that Earth is wrapped in a powerful protective shield. Charged particles from the Sun hurtle toward our planet at extreme speeds, but Earth’s magnetic field deflects and guides them along invisible pathways. As they funnel into the upper atmosphere, their energy is released as waves of light. Without this magnetic shield, Earth would be exposed—and life as we know it wouldn’t be possible.

Auroras danced across Alaska’s sky last night.😮🌌 A breathtaking sign that Earth is wrapped in a powerful protective shield. Charged particles from the Sun hurtle toward our planet at extreme speeds, but Earth’s magnetic field deflects and guides them along invisible pathways. As they funnel into the upper atmosphere, their energy is released as waves of light. Without this magnetic shield, Earth would be exposed—and life as we know it wouldn’t be possible.

Night Sky Today

24,198 Aufrufe • vor 5 Monaten

Most of us grew up seeing simplified diagrams of the Hubble Space Telescope and assumed the James Webb Space Telescope follows a similar path around Earth. In reality, it operates in a very different region of space. It is not orbiting our planet in the traditional sense but instead travels around a point about 1.5 million kilometers away known as the Sun–Earth L2 point, keeping pace with Earth as both move around the Sun. This location is often described as a gravitational balance point, but it is not truly stable or neutral. JWST does not sit still there; it follows a controlled orbit around L2 and requires periodic adjustments to stay on course. The result is a delicate, engineered dance between gravity and motion, where the telescope remains aligned with Earth while staying far from its heat and light, allowing it to observe the universe with extraordinary clarity.

Most of us grew up seeing simplified diagrams of the Hubble Space Telescope and assumed the James Webb Space Telescope follows a similar path around Earth. In reality, it operates in a very different region of space. It is not orbiting our planet in the traditional sense but instead travels around a point about 1.5 million kilometers away known as the Sun–Earth L2 point, keeping pace with Earth as both move around the Sun. This location is often described as a gravitational balance point, but it is not truly stable or neutral. JWST does not sit still there; it follows a controlled orbit around L2 and requires periodic adjustments to stay on course. The result is a delicate, engineered dance between gravity and motion, where the telescope remains aligned with Earth while staying far from its heat and light, allowing it to observe the universe with extraordinary clarity.

Cosmos Archive

31,985 Aufrufe • vor 2 Monaten

Lake Erie has become a winter wasteland. We hiked to the outer harbor breakwall tonight for sunset in sub zero temperatures. As luck would have it a 20’ snow drift gave us access to scale the ice encased structure. The view from the top of the wall was just incredible. #NYwx

Lake Erie has become a winter wasteland. We hiked to the outer harbor breakwall tonight for sunset in sub zero temperatures. As luck would have it a 20’ snow drift gave us access to scale the ice encased structure. The view from the top of the wall was just incredible. #NYwx

BuffaloSnowKing

23,409 Aufrufe • vor 5 Monaten

Rachel Reeves is expected to approve a third runway at Heathrow airport despite the fact it would wreck the country's climate ambitions and is highly unlikely to result in any GDP 'growth'. Brilliant...

Rachel Reeves is expected to approve a third runway at Heathrow airport despite the fact it would wreck the country's climate ambitions and is highly unlikely to result in any GDP 'growth'. Brilliant...

The Green Party

97,527 Aufrufe • vor 1 Jahr

Because the Rockefellers figured out… That having the trust own life insurance against all the trustees and beneficiary’s was the ingenious way to continue pumping money into the family without working for it Just taking advantage of the life insurance payouts as one beneficiary would pass away, their insurance would get paid out to the trust and the family would get the benefits And this continues over and over and over again because all you need is to have more children and add them on as beneficiaries to the trust.. once the wealth was created, they just built a method to keep it flowing forever. ~ Richard Garcia ✨🙌🏾💫

Because the Rockefellers figured out… That having the trust own life insurance against all the trustees and beneficiary’s was the ingenious way to continue pumping money into the family without working for it Just taking advantage of the life insurance payouts as one beneficiary would pass away, their insurance would get paid out to the trust and the family would get the benefits And this continues over and over and over again because all you need is to have more children and add them on as beneficiaries to the trust.. once the wealth was created, they just built a method to keep it flowing forever. ~ Richard Garcia ✨🙌🏾💫

🧬Maxpein🧬

631,722 Aufrufe • vor 5 Monaten

Richard Garcia: "Because the Rockefellers figured out… that having the trust own life insurance against all the trustees and beneficiary’s was the ingenious way to continue pumping money into the family without working for it." "Just taking advantage of the life insurance payouts as one beneficiary would pass away, their insurance would get paid out to the trust and the family would get the benefits." "And this continues over and over and over again because all you need is to have more children and add them on as beneficiaries to the trust.." "Once the wealth was created, they just built a method to keep it flowing forever."

Richard Garcia: "Because the Rockefellers figured out… that having the trust own life insurance against all the trustees and beneficiary’s was the ingenious way to continue pumping money into the family without working for it." "Just taking advantage of the life insurance payouts as one beneficiary would pass away, their insurance would get paid out to the trust and the family would get the benefits." "And this continues over and over and over again because all you need is to have more children and add them on as beneficiaries to the trust.." "Once the wealth was created, they just built a method to keep it flowing forever."

illuminatibot

105,292 Aufrufe • vor 2 Monaten

True story.. we had a mean goat on the farm.. we never allowed it out of the pasture. If you went walking it would always try to knock the heII out of you. It got out one time and as grandma was walking to her massive boat of a Buick to go to church it snuck up and rammed her hard enough to break her hip.. no one on earth seen that goat ever again ☠️🪦

True story.. we had a mean goat on the farm.. we never allowed it out of the pasture. If you went walking it would always try to knock the heII out of you. It got out one time and as grandma was walking to her massive boat of a Buick to go to church it snuck up and rammed her hard enough to break her hip.. no one on earth seen that goat ever again ☠️🪦

Bulldog 🏈 🇺🇸

653,546 Aufrufe • vor 7 Monaten

A Bolt driver and a passenger got into a physical altercation over the final cost of the ride after disagreeing on the fare The driver refused to accept the fare of GH¢ 1, stating that it was too low as the trip was a lengthy one. The passenger argued that he would only pay the price on the app and that the driver would have taken the money even if the fare were set at $1 million.

A Bolt driver and a passenger got into a physical altercation over the final cost of the ride after disagreeing on the fare The driver refused to accept the fare of GH¢ 1, stating that it was too low as the trip was a lengthy one. The passenger argued that he would only pay the price on the app and that the driver would have taken the money even if the fare were set at $1 million.

SIKAOFFICIAL🦍

1,765,210 Aufrufe • vor 3 Jahren

hobi: "the pride of Gwangju is j-hope, isn't it?" soobin: "Of course!!! Would it be okay if I sell you to the citizens a little, hyung?" hobi: "as much as you want!!!"

hobi: "the pride of Gwangju is j-hope, isn't it?" soobin: "Of course!!! Would it be okay if I sell you to the citizens a little, hyung?" hobi: "as much as you want!!!"

jayvee

34,169 Aufrufe • vor 11 Monaten

What would happen to your body in the Sun? The Sun would obviously incinerate you instantly, since its surface temperature is 5,499 °C (although the Sun doesn’t actually have a surface — that’s what they call the layer between its core and corona). However, “instantly” is a relative term. Physicist Randall Munro, a former NASA employee, believes that if you were teleported to the Sun for one nanosecond (a billionth of a second) and then returned, you would remain unharmed. Your skin would receive five orders of magnitude less heat than from touching a butane torch for a second, so you wouldn’t even feel anything. But if you were teleported closer to the core, where the temperature reaches 14,999,727 °C, you would evaporate in one femtosecond (one quadrillionth of a second).

What would happen to your body in the Sun? The Sun would obviously incinerate you instantly, since its surface temperature is 5,499 °C (although the Sun doesn’t actually have a surface — that’s what they call the layer between its core and corona). However, “instantly” is a relative term. Physicist Randall Munro, a former NASA employee, believes that if you were teleported to the Sun for one nanosecond (a billionth of a second) and then returned, you would remain unharmed. Your skin would receive five orders of magnitude less heat than from touching a butane torch for a second, so you wouldn’t even feel anything. But if you were teleported closer to the core, where the temperature reaches 14,999,727 °C, you would evaporate in one femtosecond (one quadrillionth of a second).

Black Hole

16,808 Aufrufe • vor 1 Jahr