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Space Exploration

Europe’s Ariane 6 rocket is on the verge of being launched. The following explanation will outline the reasons why this matter is significant

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Soon, Europe will be able to go into space on its own again, as Ariane 6 is set to launch for the first time this summer. We’ll let you know soon, but it’s likely to be between the middle of June and the end of July. A lot of people in Europe and beyond are scared because a lot is riding on this.

The European Space Agency (ESA) is getting a new rocket called Ariane 6. It will replace Ariane 5, which was very useful. From 1996 to 2023, Ariane 5 made 117 launches, and 112 of them were successful. Ariane 5 launched JWST into orbit. Since Arianespace produced Ariane 6, it has a lot of history to live up to and overcome. It will be taller than Ariane 5, but it will be lighter, and it will cost less to launch each time.

“The Ariane 5 rocket was Europe’s main way to send heavy and medium-sized satellites into space.” The Ariane 6 will be more up-to-date, less expensive, and able to do more. “That gives it more freedom to leave satellites in different orbits,” said Dr. Josef Aschbacher, Director General of the ESA.

“Every day, satellites help us with navigation, communication, and watching the Earth. But we also use the satellites that we send into space on our Ariane rockets to learn more about the universe.”

Coming up are missions to find habitable worlds, build X-ray observatories, and chase comets
ESA will use Ariane 6 for a variety of upcoming exciting missions. It will look for habitable worlds around stars like the Sun when it launches in 2026. It is called PLATO, which stands for planetary transits and oscillations of stars. The Atmospheric Remote-Sensing Infrared Exoplanet Large- Survey (ARIEL) mission is smaller but related. It will take its time to study the atmospheres of about 1,000 known worlds, building on the ground-breaking work that JWST is already doing.

ARIEL and its companion mission, Comet Interceptor, are set to take off in 2029. At first, the spacecraft won’t do much. It will just stay in space, far from Earth. But if a comet from the edge of the solar system or even one from between the stars gets close, it will be sent out to study the object that hasn’t been found yet. It was definitely a one-of-a-kind mission.

LISA and ATHENA live further in the future, but they have a lot of hopes for the future. LISA will be the first space observatory for gravitational waves. It will measure the vibrations in space-time in a way that we can’t do on Earth or even the Moon. The Advanced Telescope for High-Energy Astrophysics (ATHENA) will replace the following generation of X-ray observatories. It is expected to be 10 times better than the current ones. NASA is slowly cutting back on funding for its Chandra X-ray observatory, so 2035 can’t come fast enough.

“These missions will be sent off by Ariane 6,” said Dr. Aschbacher. “We are now getting ready for the next one, which is PLATO.” The big ones are definitely LISA and ATHENA, which are coming out in ten years. That’s what ESA is doing to help us understand the universe and figure out its mysteries. The Ariane 6 rocket will be needed to put those telescopes into orbit.

A future vehicle with a crew?
The Ariane 6 will launch more times than the Ariane 5. It will make sure that people can go to space on a regular basis, Dr. Aschbacher said, but his hope for this rocket is in the recently agreed-upon cargo transport vehicle. At the Space Summit between the European Union and ESA last November, a plan was made to have a reusable cargo vehicle carrying goods to and from the International Space Station by 2028. This vehicle could be converted into a crewed one after showing that it is safe and reliable.

“Right now, we don’t have this ability to re-enter Europe.” Without a doubt, this vehicle is important, and we’d like to improve this technology, which is a big step forward in exploration. This could become a crewed vehicle after it has flown a few times to make sure it is reliable and works well. “Of course that means for astronauts,” Dr. Aschbacher said with great excitement. But he was careful to say that the dream hasn’t thought through how projects are agreed upon and paid for in ESA yet.

“Just to be clear, this hasn’t been decided yet.” “I would need the member states to agree to this for it to happen,” he said. “This cargo or maybe crew vehicle would also be sent into space by Ariane 6 depending on how things go.” We’re not quite there yet, but this is how we think Ariane 6 could continue to grow.

Two types of the heavy-lift rocket Ariane 6 will be made: the 62, which has two boosters, and the 64, which has, you guessed it, four boosters. Both will be used to send things into geosynchronous transfer orbit, low-Earth orbit, and even further. The Ariane 6 upper stage will have a new Vinci engine that can be turned on and off. This will allow satellites or payloads to be put into any orbit that is needed.

An Ariane 6 and SpaceX’s Falcon 9 and Falcon Heavy have been compared a lot with the goal of letting businesses go into space. Ariane 6 can’t be used again, but compared to Ariane 5, it cuts costs by almost half. Launches on the Falcon fleet usually have a financial edge.

The edge of Ariane 6 might be in how much it can carry. Falcon Heavy’s expendable version, which costs more than the Ariane 64, can carry more cargo than the Ariane 64. For the version that can be used more than once, the fuel needed to safely bring back the rockets and booster cuts into the payload. A rocket must have enough thrust to carry its own weight, its fuel, and everything it needs to carry.

“Putting together a rocket is not simple; it takes a lot of teamwork.” “When I became Director-General of ESA three years ago, I looked at the progress of the [Ariane 6] project and saw that we had a lot of issues,” Dr. Aschbacher told. “Really, I spent 60% of my time with many team members getting the development of Ariane 6 back on track with the help of our industry partners.” We were able to solve all of the technical issues, which makes me very proud and happy.

Europe will soon have a whole new way to get to space after the launch in just a few weeks. But ESA isn’t just sitting back and waiting to see how Ariane 6 grows. The agency is already looking for the next launcher, which could be ready by the end of the 2030s.

“The next rocket after Ariane 6 will, of course, be reusable, which will cut costs even more and make it more useful for the European space industry and for everyone else.” A launcher may sound very complicated and technical, but it is useful for everyone. It sends solons into space. Not a launcher, not a space. There is no space, no way to connect to the Internet from space, no navigation systems, and no ways to watch Earth. This is really the most important thing that makes our standard of living possible. Dr. Aschbacher

It will take off from the European Space Port of Kourou in French Guiana, which is in South America and is part of France. On its first trip, it will carry many things, including a small satellite called “the witness” that will record the whole flight, from launch to deorbit and burn. The ESA’s newest space workers planned and constructed it.

As Editor here at GeekReply, I'm a big fan of all things Geeky. Most of my contributions to the site are technology related, but I'm also a big fan of video games. My genres of choice include RPGs, MMOs, Grand Strategy, and Simulation. If I'm not chasing after the latest gear on my MMO of choice, I'm here at GeekReply reporting on the latest in Geek culture.

Astronomy

Witness the rare celestial event of Mars and Jupiter reaching their closest proximity in the sky this week, a phenomenon that will not occur again until 2033.

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Mars and Jupiter will be only 0.3 degrees apart in the sky on August 14. From our point of view, this passage is very close. If you miss it, you won’t be able to see another one until 2033.

When two objects pass each other in the sky from our point of view, this is called a conjunction. Every time two planets came together, the closer one would block out the other because they would all be moving in a perfectly flat plane. The orbits of the planets are slightly different from those of the other planets, though, so they move slightly to the north and south of each other. Every time, that gap is a different size.

When two things happen close together, the results are especially stunning. Jupiter and Saturn were close enough to each other in 2020 that they could be seen in the same field of view through a telescope. This is a treat for people who like to observe the sky.

Being 0.5 degrees wide, the full moon will fit in any view that can hold the whole moon. This pair will also look good before and after the full moon.

But even with the naked eye, a close conjunction can make the sky look even more amazing. The contrast between the red of Mars and the white of Jupiter will be especially striking. However, Mars’ brightness changes a lot. When it’s at its brightest, it’s about the same brightness as Jupiter. Right now, it’s 16 times less bright. They are so bright that, unless there are clouds, you should be able to see them from all but the dirtiest cities.

Most people in the world will miss this sight, though, because they can’t see the pair of planets in the evening from anywhere on Earth. The exact time they rise depends on where you live, but it’s usually between midnight and 3 am. To see this, you will mostly need to get up before astronomical twilight starts so that you have time to get through the thickest part of the atmosphere.

For people in Europe, Africa, west Asia, and the Americas, the closest time will be 14:53 UTC, which is during the day. The mornings before and after, though, will look almost as close.

Mars and Jupiter meet about every two and a half years, but the most recent one was almost twice as far away and could only be seen in the morning. In 2029, the gaps will be just under two degrees. The next one will be even wider, at more than a degree.

When planets are close to each other, that doesn’t always mean that their distance from each other is very small. Mars has been around the Sun for 687 days, but it is now less than 100 days past its perihelion, which means it is closer than usual. Even though Jupiter is a little closer than usual, it’s not really that close. To be as close as possible to each other, Mars has to be at its farthest point, and Jupiter has to be at its closest point. So this one is not unusual.

But if you want to see something beautiful, you will have to wait more than nine years to see it again.

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Space Exploration

World’s first implantation of a titanium heart harnessing maglev technology

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When looking for alien civilizations, it can be hard to know what to look for. During the search, we have mostly looked for signals and signs that we would send out (either on purpose or by accident) because we think that aliens will use similar technology since they can use the same physics.

It makes sense to do that, but it’s not the best thing to do. As we’ve seen over the last few hundred years on Earth, intelligent societies can quickly get rid of old technology that can be found as they learn more about the universe. As a clear example, we quickly switched from communicating with analog signals to digital ones. Of course, analog signals in the range we used for communication wouldn’t work very well on alien planets. However, it’s possible that alien civilizations could go “radio quiet” in about 100 years, which would make it even harder to find them.

Scientists have thought about what kind of signal a more advanced civilization might send and how advanced the technology would have to be in order to send it.

Even though it’s just a guess, we have some ideas about what kind of signal would make sense and what the message should say to make it clear that it comes from a smart being.

At that time, the plan was to study a region around 1.42 GHz, which is a well-known frequency where neutral hydrogen gives off radiation in interstellar space. Bryan Brzycki, a graduate student in astronomy at UC Berkeley, told Universe Today more about this. “Because this natural emission is common in the galaxy, it is thought that any intelligent civilization would know about it and might choose to send signals at this frequency to increase their chances of being found.” In the years since then, radio SETI has grown in every way, especially as technology has quickly improved.

Transmitting signals across the galaxy or universe, especially persistent signals that would maximize our likelihood of being detected, necessitates a substantial amount of energy, surpassing the capabilities of human beings. In 1963, Soviet astronomer Nikolai Kardashev endeavored to quantify the magnitude of energy required for transmitting signals containing information, as well as the corresponding levels of technological development that civilizations would need to achieve in order to accomplish this.

Kardashev categorized these theoretical civilizations into three classifications, depending on their capacity to exploit energy from their environment.

Type I civilizations are those that possess the capability to fully utilize the total energy resources of their planet, estimated to be approximately 4 x 1019 erg per second, for their own objectives. Type II civilizations possess the capability to exploit the energy emitted by their star, such as through the construction of Dyson Spheres. These are hypothetical colossal structures specifically designed to enclose stars and harness their energy. Type III civilizations refer to extraterrestrial civilizations that possess the ability to utilize the energy resources of their entire galaxy.

Despite the fact that Type II and III civilizations have significantly high energy production levels, Kardashev estimated that humanity would take approximately 3,200 and 5,800 years to reach those levels, based on Earth’s annual energy production growth rate of 1 percent. In 2020, a comprehensive scale was proposed that introduces the concept of a Type IV civilization capable of harnessing the energy of the entire observable universe. Based on our energy consumption, this team asserts that humans are presently classified as a Type 0.72 civilization.

According to Kardashev, it is highly improbable to detect Type I civilizations due to their relatively small but significantly greater energy output compared to our own. However, a Type I civilization, similar to ours, could potentially detect signals emitted by Type II and Type III civilizations using conventional radio telescopes, although they would not be able to respond to them. The premise of the work is that extraterrestrial civilizations would be transmitting scientific knowledge well ahead of our own, with the purpose of being detected by less advanced civilizations. However, this strategy may not be advisable for any civilization that seeks to ensure its survival.

Nevertheless, the Kardashev scale provides insight into the types of civilizations that possess the ability to transmit signals that we may soon have the capacity to detect. If advanced civilizations indeed exist (considering the immense expanse of the universe and its prolonged existence, this supposition is plausible), it would provide us with additional avenues of exploration, such as the search for colossal megastructures employed for energy extraction.

While we possess a relatively accurate understanding of our current and potential abilities, the universe has been in existence for significantly longer durations. Examining the capabilities of an advanced extraterrestrial civilization can provide insights into our own potential future possibilities. If our search of the celestial realm yields no evidence of Type III civilizations capable of harnessing energy on a galactic scale—a phenomenon that has yet to occur—it could indicate the existence of an obstacle that prevents intelligent species from attaining such an advanced stage. This obstacle, known as the Great Filter, may be looming in our future.

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Physics

An interest They stepped on a rock and found something on Mars that had never been seen before

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NASA’s curiosity has been looking into an interesting part of Mount Sharp for the past 10 months. It shows signs of a violent watery past, and chemical tests have shown that it contains many minerals, such as sulfates. The rover also broke open a rock by accident as it moved around. And inside it were crystals of pure sulfur.

On Mars, people had never seen pure sulfur before. Even though sulfates contain sulfur, there isn’t a clear link between how those molecules form and how the pure crystals form. Crystals of elemental sulfur can only form in a few different situations. And none of those were thought to happen in this area.

To find a field of stones made of pure sulfur is like finding an oasis in the middle of the desert, said Ashwin Vasavada, the project scientist for Curiosity at NASA’s Jet Propulsion Laboratory. “That thing shouldn’t be there, so we need to explain it.” It’s so exciting to find strange and unexpected things when exploring other planets.

The Gediz Vallis channel is the name of the area that Curiosity is exploring. A groove across Mount Sharp has been interesting for a long time, even before the rover started climbing it in 2014. From space, scientists could see that there were big piles of debris. But it wasn’t clear what caused them. Was it landslides or floodwaters from a long time ago that moved the stuff along the channel?

The answer has been found through curiosity. Some column A and some column B. Water-moved rocks are smoother and rounder. Sharp and angular are those that dry avalanches moved. There are both kinds of rocks in the mounds.

“This was not a quiet time on Mars,” said Becky Williams, a scientist from Tucson, Arizona, who works for the Planetary Science Institute and is the deputy principal investigator of Mastcam on Curiosity. “There was a lot of exciting stuff going on here.” We expect a number of different flows to happen down the channel, such as strong floods and flows with lots of rocks.

Curiosity is still looking into the Gediz Valley. When the ball rolls around and shows off its unique features, we can get very excited about the science being done here.

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