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The planet Neptune; Everything you need to know

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Neptune
Neptune, the farthest planet from the Sun, is one of the two ice giants of the solar system, along with Uranus.

The planet Neptune; Everything you need to know

Neptune is the eighth planet of the solar system and the farthest planet from the sun. But it is not the coldest planet. This blue gas giant of the solar system is significantly larger than Earth and has 17 times the mass of Earth. Neptune’s rocky core is surrounded by a mixture of water ice, ammonia, and methane.

Table of Contents
  • What does the planet Neptune symbolize?
  • Distance from Earth to Neptune
  • How was Neptune formed?
  • Characteristics of Neptune
  • moons of Neptune
  • Neptune’s rings
  • Interesting facts about the planet Neptune
  • Why is Neptune blue?
  • Neptune’s Diamond Rain
  • The stormiest planet
  • How cold is Neptune?
  • The strange temperature of Neptune
  • Neptune’s solid core is roughly the same size as Earth
  • Neptune has migrated to its current position
  • Life on Neptune is unlikely
  • Discoveries of Neptune
  • Journey to Neptune
  • Photo of the planet Neptune
  • Conclusion

What does the planet Neptune symbolize?

The ice giant Neptune was the first planet to be discovered based on mathematical calculations. This planet was discovered in 1846 based on the predictions of astronomers such as Urban Le Verrier and Johann Galle. The name Neptune is derived from the name of the Roman god of the sea, which was suggested by Le Verrier.

Distance from Earth to Neptune

The distance between Neptune and Earth is between 3.4 billion and 7.4 billion kilometers, depending on the position of the two planets in their orbits. Voyager 2 took 12 years to reach Neptune. This probe traveled at an average speed of 68,000 kilometers per hour, which is much faster than the speeds that humans have traveled so far.

Voyager photo of NeptuneVoyager 2 captured this image in 1989.

How was Neptune formed?

About 4.5 billion years ago, the planet Neptune turned into an ice giant due to the accumulation of gas and dust due to gravity. This planet, like its neighbor Uranus, was probably at a closer distance from the Sun and then moved to the outer solar system about 4 billion years ago.

Characteristics of Neptune

Most of Neptune is made up of water, ammonia, and methane. The planet does not have a solid surface but has a solid core like Earth. Neptune is an ice giant along with Uranus. This nickname distinguishes Neptune from gas giants such as Jupiter and Saturn because Neptune and Uranus have higher amounts of ice-forming molecules.

Most of Neptune’s visible atmosphere consists of hydrogen (more than 80%) and helium (15%). A small amount of methane and other molecules such as ethane, acetylene, and some other hydrocarbons are found in this section.

Inside NeptuneNeptune’s internal structure: (1) clouds above the atmosphere (2) atmosphere: a mixture of hydrogen, helium and methane (3) mantle: including water ice, ammonia, and methane (4) rocky core: silicate and iron, nickel

However, the deeper we go into this planet, the more its composition changes. Based on the overall density of Neptune, heavier elements are located in its depths; Therefore, ten to twenty percent of the total composition of Uranus and Neptune includes hydrogen and helium, and 80 to 90 percent of those elements are heavier. The heavier elements are methane, ammonia, and water, as well as other elements that make up the rocky and metallic parts.

Neptune is the fourth largest planet in the solar system with a radius of 24,622 km. One Neptune day is equal to 16 Earth hours (one day is Neptune’s rotation around itself or spin). One Neptune year is equal to 165 Earth years. Sometimes the distance of Neptune from the Sun is further than the distance of the dwarf planet Pluto. Pluto’s highly irregular, elliptical orbit interferes with Neptune’s orbit for twenty years every 248 Earth years. As a result of this shift, Pluto is closer to the Sun than Neptune. This interference occurred for the last time between 1979 and 1999. However, Pluto never collides with Neptune.

Moons of Neptune

Neptune has 14 confirmed moons. The largest moon of this planet is Triton, which rotates in the opposite direction to the spin of Neptune. This reverse orbit shows that Triton was not always associated with Neptune and researchers believe that it was trapped by Neptune’s gravity from the Kuiper belt almost millions of years ago. Triton is the only spherical moon of Neptune and the other 13 moons of this planet have irregular shapes.

The surface temperature of Triton reaches minus 235 degrees Celsius and this feature makes it one of the coldest places in the solar system. However, Voyager 2 discovered glaciers that spewed ice up to 8 km away, indicating Triton’s hot interior. Scientists are also investigating the possibility of an underground ocean on this icy moon. Scientists discovered the existence of seasons in Triton in 2010.

Nereid is another moon of Neptune, due to its special orbit, it is one of the strangest moons in the solar system. This moon can move close to Neptune at a distance of 1.4 million kilometers to a distance of 9.7 million kilometers.

Triton, Neptune's moonThis image of Triton was captured by Voyager 2 in 1989.

Neptune’s rings

Last year, the James Webb Space Telescope captured the clearest image of Neptune’s rings. Neptune is surrounded by strange rings that are not solid and contain thick, glowing clumps of dust. There are at least five rings around Neptune, and their names are Galle, Laurier, LaSalle, Arago, and Adams. These rings are relatively young and have a short life. Ground-based observations show that Neptune’s rings are much more unstable than previously thought.

Neptune's ringsThe James Webb Space Telescope released the clearest image yet of Neptune’s rings in September 2022.

Interesting facts about the planet Neptune

Why is Neptune blue?

Neptune’s surface clouds appear bright blue in part due to the absorption of red light by methane in the planet’s atmosphere. Neptune has clouds that are mainly composed of icy methane, in fact, icy methane particles are the main cause of this planet’s blue color.

Clouds of NeptuneCloud streaks on the surface of Neptune. This image was captured by the Voyager 2 probe. The width of cloud streaks varies from 50 to 200 km.

Neptune’s Diamond Rain

The planets Neptune and Uranus are famous for their diamond showers. This phenomenon occurs due to the high pressure of the atmosphere of these planets, which is 200 thousand times that of Earth. This pressure breaks the methane in the atmosphere and releases carbon. The carbon then forms long chains and diamond-like crystal patterns. Diamond fragments fall onto the mantle and then evaporate due to mantle conditions. The innermost part of the mantle of these planets has an approximate temperature of 6727 degrees Celsius and an approximate pressure of 6 million times that of the Earth.

Neptune's Diamond RainThis visualization shows Neptune’s diamond shower.

The stormiest planet

Neptune is the windiest planet in the entire solar system. Despite being so far away and receiving little energy from the Sun, Neptune’s winds can be three times stronger than Jupiter’s and nine times stronger than Earth’s. These winds move frozen methane clouds across the surface of the planet at speeds of over 2,000 km/h. This is while the speed of the strongest winds on earth reaches only 400 km/h.

In 1989, a large oval-shaped storm called the Great Black Spot appeared in Neptune’s southern hemisphere. This storm was so big that it could contain the entire globe. The Great Black Spot has disappeared, but new spots have appeared in various parts of Neptune.

big black spotThe Great Black Spot as seen by the Voyager 2 probe

How cold is Neptune?

The temperature of Neptune’s atmosphere reaches minus 225 degrees Celsius. Although Neptune is expected to be the coldest planet as the farthest planet from the Sun, Uranus and Neptune have almost the same temperature, and some regions of Uranus are even colder than Neptune.

The strange temperature of Neptune

Neptune's temperature changesTemperature changes of Neptune in different years

In 2019, NASA discovered evidence of Neptune’s strange temperature changes. Using thermal cameras, researchers tracked the average temperature of the planet. Since changes were first recorded in 2003, Neptune has cooled over time. The temperature of Neptune’s southern hemisphere has decreased by 8.7 degrees Celsius between 2003 and 2018. But this trend seems to have reversed between 2018 and 2020 and the temperature has suddenly increased up to 10.6 degrees Celsius. The reason for these changes is not clear, but one of the possible reasons is the seasonal changes, each lasting 40 years.

Neptune’s solid core is roughly the same size as Earth

Under the thick atmosphere of Neptune, it is speculated that there is a solid core about the size of the planet Earth. Despite the lack of data, Neptune’s core is likely composed of heavier elements such as iron, nickel, and silicates.

Neptune has migrated to its current position

Another fascinating fact about Neptune is that it probably moved to its current position early in its formation. This attitude goes back to the exact mechanism of the formation of Neptune. According to researchers, this planet probably formed at a closer distance from the sun and then moved.

Life on Neptune is unlikely

Most scientists consider the possibility of life on Neptune to be small or impossible. Neptune’s conditions are very different from those of a planet like Earth, and the absence of liquid water would completely disrupt the existence of life as we know it. On the other hand, the atmosphere and surface of Neptune experience new temperatures and pressure, and this arrangement of the planet Neptune is a harsh environment for the formation of any kind of complex or primitive life.

Cassini image of NeptuneThe Cassini spacecraft released this image of Neptune in August 2017.

Discoveries of Neptune

Scientists discovered Neptune in 1846 after calculating the orbit of Uranus. According to these calculations, an unknown planet was influencing the gravity of Uranus. It is not possible to see Neptune with the naked eye, but researchers were able to confirm the existence of this planet with a telescope. Astronomer Galileo Galilei was one of the first people to identify Neptune as a space body, however, because of its slow motion, he thought Neptune was a star.

Journey to Neptune

Voyager 2 is the only land probe that managed to visit Neptune. This probe released the first images of the blue planet in 1989 on its way out of the solar system. Neptune appears blue in these images due to methane in the atmosphere.

In 2020, NASA talked about the possibility of launching a new mission called Trident to visit Triton, Neptune’s largest moon. In general, learning about ice-giant planets like Neptune is important for several reasons. First of all, the extreme atmospheric conditions and long seasonal intervals of the ice giants provide a unique opportunity to understand the physics of weather and climate. In addition, these planets help us learn more about the formation of the solar system. Understanding Uranus and Neptune will also help to better understand the formation of the planets and how they differ from Jupiter and Saturn.

From a more general perspective, these ice giants are likely representative of the general group of planets common in the galaxy. According to the survey of exoplanets that have been discovered in the past years, exoplanets the size of Neptune are one of the most common planets. By understanding the formation and characteristics of ice giants, scientists hope to gain a better perspective of other exoplanets.

Photo of the planet Neptune

Voyager 2 is the only probe that has captured clear images of Neptune. However, Hubble and James Webb space telescopes also released images of this blue giant. In 2016, using the Hubble Space Telescope, scientists discovered a new black spot on Neptune, which is considered the first stormy spot in the 21st century.

Hubble Space Telescope photo of NeptuneHubble Space Telescope photo of Neptune

Conclusion

Neptune is the eighth planet in the solar system and the farthest planet from the sun. This blue planet has 14 moons and five unstable rings. The speed of Neptune’s winds reaches 2000 kilometers per hour, which is several times the speed of the strongest winds on Earth. Voyager 2 is the only probe that visited Neptune and captured beautiful images of this planet. Triton, Neptune’s largest moon, is also a mysterious source with fascinating geyser-like features that scientists have proposed projects to investigate.

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Why is it still difficult to land on the moon?

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More than half a century after the first spacecraft to reach the moon, a successful landing on Earth’s only moon remains a challenge for space agencies and private companies.

Why is it still difficult to land on the moon?

This year, the private company Spacel and the Indian Space Organization both met tragic ends when they tried to land their spacecraft on the surface of the moon. Despite the astonishing leaps made in recent decades in computing, artificial intelligence and other technologies, it seems that landing on the moon should be easier now; But recent setbacks show that we still have a long way to go with safe and trouble-free landings on the surface of Earth’s only moon.

50 years after sending the first man to the surface of the moon, the question arises as to why safely landing a spacecraft on Earth’s nearest cosmic neighbor is still a difficult task for space agencies and private space companies. Stay with Zoomit to check the answer to this question.

Why is the lunar landing associated with 15 minutes of fear?

Despite the complexities of any space mission, sending an object from Earth into orbit around the moon today is easy. Christopher Riley, the director of the documentary film In the Shadow of the Moon produced in 2007 and the author of the book Where We Stood (2019), both of which are about the history of the Apollo 11 mission, explained the reasons for the difficulty of landing on the moon in an interview with Digital Trends. is According to him: “Today, the paths between the Earth and the Moon are well known, and it is easy to predict them and fly inside them.”

Chandrayaan-2
Chandrayaan 2 mission launch

However, the real challenge is getting the spacecraft out of orbit and landing it on the lunar surface; Because there is a delay in the communication between the Earth and the Moon, and the people in the control room who are present on the Earth cannot manually control the spacecraft in order to land it safely on the Moon. As a result, the spacecraft must descend automatically, and to do so, it will fire its descent engines to slow its speed from thousands of kilometers per hour to about one meter per second, in order to make a safe landing on the lunar surface.

For this reason, the director of the Indian Space Research Organization (ISRO), who was trying to land the Vikram lander last month, described the final descent of the spacecraft as “frightening 15 minutes”; Because as soon as the spacecraft enters the landing stage, the control of its status is out of the hands of the mission control members. They can only watch the spacecraft land and hope that everything goes according to plan, that hundreds of commands are executed correctly, and that the automatic landing systems gently bring the spacecraft closer to the surface of the moon.

The Great Unknown: The Landing Surface

One of the biggest challenges in the final descent phase is identifying the type of landing site. Despite the availability of instruments such as the Lunar Reconnaissance Orbiter (LRO) that can capture amazing views of the lunar surface, it is still difficult to know what kind of surface the spacecraft will encounter when it lands on the moon.

Beresheet crash site
Left: Breshit crash site. Right: The ratio of the before and after images highlights the occurrence of minor changes in surface brightness.

Leonard David, author of Moon Fever: The New Space Race (2019) and veteran space reporter, says:

The Lunar Reconnaissance Orbiter is a very valuable asset that has performed really well over the years; But when you get a few meters above the surface of the moon, complications appear that cannot be seen even with the very powerful LRO camera.

Even today, despite the imaging data available, “some landing sites still have unknown remains,” Riley says. He notes that the Apollo 11 mission included an advantage that today’s unmanned landers lack, which is the presence of an astronaut’s observer’s eyes that can closely observe the surface of the spacecraft’s landing site. As you probably know, in the mission that led to the landing of the first man on the surface of the moon, the Eagle computer was guiding the spacecraft to a place full of boulders; But to avoid hitting the rocky surface of the moon, Armstrong took control of the spacecraft himself and landed it on a flat surface.

Apollo 11 / Apollo 11

The uneven surface of the landing site had caused many problems in previous lunar missions such as Apollo 15. In this mission, the astronauts were told that as soon as the spacecraft touched the surface of the moon, they should turn off the engines to prevent dust from being sucked in and the risk of a return explosion. But the Apollo 15 spacecraft landed in a crater, and because of this, one of its legs came into contact with the surface earlier than the others. When the crew shut down the engines, the spacecraft, moving at a speed of 1.2 meters per second, experienced a hard landing. The lander landed at an oblique angle, and although it eventually landed safely, it nearly overturned, causing a fatal disaster.

  • Half a century after Apollo 11; How did the great human leap happen?
  • dust storms; The nightmare of space missions to the moon

The difficult landing of Apollo 15 introduced another complicating factor in lunar landings: lunar dust. The Earth’s moon is covered with dust that is thrown into the air by any movement and sticks to everything it comes in contact with. As the spacecraft approaches the surface of the moon, huge plumes of dust are kicked up that limit the field of view and endanger the spacecraft’s electronics and other systems. We still do not have a solution to deal with the dust problem.

An achievement that has been achieved before

Another reason why the moon landing remains a challenge is that gaining public support for lunar projects seems difficult. Referring to Neil Armstrong and Buzz Aldrin, the two astronauts who walked on the moon during the Apollo 11 mission, David says, “We convinced ourselves that we had sent Neil and Buzz [to the surface of the moon]; “As a result, when it comes to lunar missions, people may say we’ve been there before and we’ve had this success.”

Apollo 11 / Apollo 11

But in reality, our understanding of the moon is still very little, especially in relation to long-term missions. Now, with a 50-year gap between the Apollo missions and NASA’s upcoming Artemis project, the knowledge gained has been lost as engineers and specialists retire. David says:

We need to recover our ability to travel into deep space. We haven’t gone beyond near-Earth orbit since Apollo 17 and since 1972. NASA is no longer the same organization that put men on the moon, and there is a whole new generation of mission operators.

The importance of redundancy

As the first private spacecraft entered into orbit around the moon, the Space project was of considerable importance; But its failure to land smoothly on the surface of the moon made the achievement of landing on the surface of the moon still remain in the hands of governments. However, we can expect more private companies, such as Jeff Bezos ‘ Blue Origin, which is developing its lunar lander, to target the moon in the future. According to Elon Musk, even the giant SpaceX Starship spacecraft, which is being built with the ultimate goal of sending a human mission to Mars , can also land on the moon.

According to David, private companies’ participation in lunar landings has advantages such as increased innovation. However, companies are under pressure to save money, and this can lead to a lack of redundancy and support systems that are essential in the event of errors and malfunctions. Lunar rovers typically include two or even three layers of support systems. David is concerned that private companies will be encouraged to eliminate these redundancies in order to cut costs and save money.

Crew Dragon
Crew Dragon SpaceX passenger capsule

“We saw Elon Musk’s Dragon capsule catch fire after a failed test on the stand,” says David, referring to the explosion of the SpaceX spacecraft in April, which had no crew on board. “This accident was kind of a wake-up call about how unpredictable the performance of spacecraft can be.” David compared the Crew Dragon incident to the Apollo 1 disaster, which killed three NASA astronauts during a test launch in 1967.

Another problem related to the lack of redundancy systems is the lack of information needed when an error occurs. As for the recent landings, it seems that the SpaceX crash was caused by human error; however, it is not clear what caused the failure of Chandrayaan 2 in the calm landing, and it is possible that without the necessary systems to record and send information to the lander, we will never find out the main reason for the failure of this mission. Without the required data, it becomes much more difficult to prevent problems from reoccurring in the future.

The future of lunar landings

Currently, many projects are underway to facilitate future moon landings. Ultimately, we need to be able to build the necessary infrastructure for a long-term stay on the moon.

Moonrise Project
Conceptual design of Moonrise technology on the moon. On the left side is the Alina lunar module, and on the right side, the lunar rover equipped with Moonrise technology melts the lunar soil with the help of a laser.

If we can make long-term stays on the moon possible, or even build a permanent base there, landing spacecraft on the lunar surface will be much easier. By constructing the landing sites, a flat, safe, and free surface of unknown debris can be created for the landing of surface occupants. For example, researchers are currently conducting research at NASA’s Kennedy Space Center to investigate the feasibility of using microwaves to melt the lunar soil (regolith) and turn it into a hard foundation so that it can be used as a landing and launch site. The European Space Agency is also investigating how to use 3D printing to create landing sites and other infrastructure on the moon.

Read more: Europa Clipper, NASA’s flagship probe was launched

Other ideas include the use of lidar remote sensing systems, which are similar to radar systems; But instead of radio waves, it uses lasers to land the spacecraft. Lidar technology provides more accurate readings and uses a network of GPS satellites to help guide the spacecraft during landing.

The problem of public support

As important as technology is, public interest and support are essential to the success of the lunar landing program. “Apollo had enormous resources that are perhaps only comparable today to China’s space program,” says Riley. “Remember that Apollo carried the best computer imaginable, the human brain.” It goes without saying that there is an element of luck involved in every landing.

Mike Pence
US Vice President Mike Pence speaking at the 50th anniversary of the Apollo 11 mission

Finally, there is the question of what kind of failure is acceptable for people. David says:

I think we have to be serious about the fact that we’re probably going to lose people. There is a serious possibility that the manned lunar lander will crash and kill the astronauts inside. The American people continued to support NASA despite the failures and bad luck of the Apollo program, But at that time there was a lot of pressure to compete with the Soviet Union. Without the bipolar atmosphere of the Cold War and the space race, would people still support missions with human lives in between?

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Europa Clipper, NASA’s flagship probe was launched

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The highly anticipated Europa Clipper probe has finally begun its long journey to uncover the mysteries of Europa, Jupiter’s moon, by launching aboard a SpaceX Falcon Heavy rocket.

Europa Clipper, NASA’s flagship probe was launched

After years of waiting, NASA’s Europa Clipper probe was finally launched on Monday at 7:36 p.m. Iran time from the Kennedy Space Center on top of SpaceX’s Falcon Heavy rocket and began a major astrobiology mission to Europa, the potentially habitable moon of Jupiter.

As SpaceX’s massive rocket powered by 27 powerful Merlin engines lifted off from pad 39A, NASA live broadcast reporter Dron Neal said, “The launch of Falcon Heavy with Europa Clipper will reveal the secrets of the vast ocean beneath the icy crust of Europa, Jupiter’s moon. It has been hidden, it will reveal.”

The engines of the two side boosters of the Falcon Heavy were shut down and separated from the central booster approximately three minutes after the flight. The central booster continued to fly for another minute, and then in the fourth minute of the launch, the separation of the upper stage from the first stage was confirmed. Finally, 58 minutes later, Europa Clipper was injected into interplanetary orbit as scheduled. A few minutes later, the mission team made contact with the probe, and people in the control room cheered and applauded.

Falcon Heavy’s unique launch

The launch of NASA’s new probe was delayed due to some mishaps. NASA and SpaceX initially planned to launch the Europa Clipper mission on Thursday, October 10; But with powerful Hurricane Milton hitting Florida’s Gulf Coast on Wednesday evening, a delay in the launch became inevitable. NASA shut down Kennedy Space Center to deal with the storm, and Europa Clipper was placed inside SpaceX’s hangar near Launch Pad 39A.

The recent launch was Falcon Heavy’s 11th flight overall and its second interplanetary mission. Also, this was the first flight of the Falcon Heavy, when all three boosters of the first stage of the rocket were deployed.

Typically, the Falcon Heavy and Falcon 9 first-stage boosters store enough fuel to perform landing maneuvers for recovery and reuse in the future; But Europa Clipper needed all the power that Falcon Heavy could provide in order to make it on its way to the Jupiter system.

A long way to the launch pad

In late 2015, the US Congress directed NASA to launch Europa Clipper using the Space Launch System (SLS), NASA’s massive rocket. SLS was still under construction at the time and was several years away from reaching the launch pad. The delay in completing the construction of this powerful rocket and NASA’s need to assign at least the first three versions of SLS to the Artemis lunar mission caused the Europa Clipper launch date to be in an aura of uncertainty.

In the 2021 House budget draft for NASA, the agency was directed to launch Europa Clipper by 2025 and, if possible, with SLS. However, due to the unavailability of the Space Launch System, NASA had to go to SpaceX’s Falcon Heavy. This decision was not without cost. As the most powerful rocket ever used in an operational mission, SLS can send Europa Clipper directly to the Jupiter system in less than three years.

Europa Clipper will use the gravitational assistance of Mars and Earth on its way to the Jupiter system

Now, even in Falcon Heavy’s fully disposable mode, the Clipper’s trip to Europe takes almost twice as long. The probe should make a flyby of Mars in February 2025 and a flyby of Earth in December 2026 to gain enough speed to reach its destination in April 2030.

Missile problems were not the only obstacles facing Europa Clipper on its way to the launch pad. For example, the rising costs of this five billion dollar probe forced NASA to cancel the construction of one of the probe’s science instruments. This instrument, named “Identification of Europa’s internal features using a magnetometer” (ICEMAG), was designed to measure Europa’s magnetic field.

Then in May 2024, NASA found that transistors similar to those used in Europa Clipper, which are responsible for regulating the probe’s electricity, were “failing at lower-than-expected radiation doses.” Following this discovery, NASA conducted more tests on the transistors and finally concluded in late August that these components could support the initial mission in the radiation-rich environment around Jupiter.

Ambitious mission to a fascinating moon

Imaging from the Europa Clipper probe over Europa, Jupiter's oceanic moon

NASA/Jet Propulsion Laboratory-Caltech

Europa Clipper is one of NASA’s most exciting and ambitious flagship missions, and it has impressive features. For example, the mission probe is the largest spacecraft NASA has ever built for a planetary mission. Europa Clipper weighed almost 6,000 kg at the time of launch and will be more than 30 meters long (bigger than a basketball court) by opening its huge solar panels in space.

Clipper’s Europa destination is also a prominent location: Europa, one of Jupiter’s four Galilean moons. The moon is covered with an icy outer shell, which scientists believe hides a vast ocean of salty liquid water. For this reason, Europa is considered one of the best places in the solar system to support alien life.

In early 2012, studies began to look for potential plumes of water rising from Europa’s surface. Some researchers theorize that those water columns and vents from which the columns protrude may contain evidence of life living beneath the moon’s icy crust. However, NASA scientists have made it clear that Europa Clipper is not looking for extraterrestrial life in Europa; Rather, this probe will only investigate the potential of the submoon water environment to support life.

“If there’s life on Europa, it’s going to be under the ocean,” Bonnie Buratti, senior Europa Clipper scientist at NASA’s Jet Propulsion Laboratory, said in September. As a result, we cannot see it.” “We will be looking for organic chemicals that are prerequisites for life on the surface of the moon,” Borrati added. There are things we can observe; such as DNA or RNA; But we don’t expect to see them. As a result, [the probe] is only looking for habitable environments and evidence for the ingredients of life, rather than life itself.”

NASA scientists have made it clear that Europa Clipper is not looking for extraterrestrial life in Europa

Europa Clipper will collect data using a suite of nine scientific instruments, including visible and thermal cameras, several spectrometers, and special equipment to identify Europa’s magnetic environment. As stated on NASA’s Europa Clipper page, the probe will help scientists achieve three main goals:

  • Determining the thickness of Europa’s ice sheet and understanding how Europa’s ocean interacts with the lunar surface.
  • Investigating the composition of Europa’s ocean to determine whether it has the materials necessary to form and sustain life.
  • Studying the formation of Europe’s surface features and discovering signs of recent geological activities; such as the sliding of crustal plates or the discharge of water columns in space.

Europa Clipper also transports Earth’s culture to the Solar System. A piece called “In Praise of Mystery: A Poem for Europe” by Edda Lemon, a famous American poet, is engraved in the artist’s own handwriting on a metal plate. In addition, the probe carries a coin-sized chip that contains the names of 2.6 million inhabitants of planet Earth.

6-year journey

Illustration of Europe Clipper over Europe

Johns Hopkins University Applied Physics

If all goes according to plan, Europa Clipper will enter Jupiter’s orbit in April 2030. When the probe gets there, it will use up 50-60% of its 2,722 kg of fuel by performing an injection maneuver for 6-8 hours.

The injection maneuver puts Europa Clipper in an elliptical orbit around the gas giant. A series of long maneuvers will then be performed to align the trajectory so that the probe can fly by Europa more than 45 times and study it closely. In fact, Europa Clipper will remain around Jupiter throughout its mission; Because according to the launch environment of Europa, it will be very dangerous for the spacecraft to go around the moon.

If all goes according to plan, Europa Clipper will enter Jupiter’s orbit in April 2030

The first flight over Europe will not take place before the spring of 2031. NASA will use the first pass to make further corrections to Europa Clipper’s trajectory in preparation for the probe’s first science mission. With the start of scientific flybys in May 2031, Europa Clipper will aim its array of sensors towards the far hemisphere from Jupiter and will approach the surface of the moon up to 25 km. The second science campaign will begin two years later, in May 2033, in the Jupiter-facing hemisphere of Europa.

The end of the Europa Clipper mission is set for September 2034. At that time, NASA will crash the spacecraft into Ganymede, another Galilean moon of Jupiter. This disposal strategy was chosen because Ganymede is considered a relatively poor candidate to host life, and the mission team wanted to make sure they did not contaminate potentially life-hosting Europa with terrestrial microbes.

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Dark matter and ordinary matter can interact without gravity!

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Dark matter and ordinary matter can interact without gravity! Dark matter, which has five times the mass of normal matter, helps hold galaxies together and explains the puzzling motions of stars. Now a new study has shown that these two substances can interact with each other without the presence of gravity.

Dark matter and ordinary matter can interact without gravity!

Why is dark matter associated with the adjective “dark”? Is it because it harbors some evil forces of the universe or hidden secrets that scientists don’t want us to know? No, it is not. Such fanciful assumptions may sound appealing to a conspiracy theorist, but they are far from the truth.

Dark matter is called dark because it does not interact with light. So when dark matter and light collide, they pass each other. This is also why scientists have not been able to detect dark matter until now; it does not react to light.

Although it has mass and mass creates gravity, this means that dark matter can interact with normal matter and vice versa. Such interactions are rare, and gravity is the only known force that causes these two forms of matter to interact.

However, a new study suggests that dark matter and ordinary matter interact in ways other than gravity.

If this theory is correct, it shows that our existing models of dark matter are somewhat wrong. In addition, it can lead to the development of new and better tools for the detection of dark matter.

Read more: There is more than one way for planets to be born

A new missing link between dark and ordinary matter

Dark matter is believed to have about five times the mass of normal matter in our universe, which helps hold galaxies together and explains some of the motions of stars that don’t make sense based on the presence of visible matter alone.

For example, one of the strongest lines of evidence for the existence of dark matter is the observation of rotation curves in galaxies, which show that stars at the outer edges of spiral galaxies rotate at rates similar to those near the center. These observations indicate the presence of an invisible mass.

Also, for their study, the researchers studied six ultra-dim dwarf (UFD) galaxies located near the Milky Way. However, in terms of their mass, these galaxies have fewer stars than they should. This means they are mostly made up of dark matter.

According to the researchers, if dark matter and normal matter interact only through gravity, the stars in these UFDs should be denser in the centers and more spread out toward the edges of the galaxies. However, if they interact in other ways, the star distribution looks different.

The authors of the study ran computer simulations to investigate both possibilities. When they tested this for all six ultra-dim dwarf (UFD) galaxies, they found that the distribution of stars was uniform, meaning that the stars were spread evenly across the galaxies.

This was in contrast to what is generally observed for gravitational interactions between dark matter and normal matter.

What causes this interaction?

The results of the simulations showed that gravity is not the only force that can make dark matter and normal matter interact. Such an interaction has never been observed before, and it could change our understanding of dark matter and dark energy.

However, this study has a major limitation. What caused the interaction between the two forms of matter is still a mystery. While the current study provides tantalizing hints of a novel interaction, its exact nature and underlying causes remain unknown. Hopefully, further research will clarify the details of such interactions.

This study was published in The Astrophysical Journal Letters.

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