Beetlejuice, a red supergiant, is this ball of boiling plasma. It’s one of the largest stars in our galaxy and one of the brightest. It’s about 500 times larger than the Sun, but Beetlejuice is pulsating, getting bigger and smaller. At its peak, it becomes 800 times its average size. If this star were a bucket, it could hold about 300 million suns despite its weight being only 17 times greater, and here, about 500 light years away, is Earth. We launch our faster-than-light spaceship and seize this opportunity. The surface of Mars is three times smaller than that of Earth, and the planet is ten times lighter. People hope to establish a colony here in the near future. Beyond Mars, we must continually wiggle. This is the asteroid belt, which contains debris and space objects of various sizes and shapes. The largest of these objects is Saturn; its surface is slightly larger than the area of Argentina, and its mass is about one percent that of the moons. The total mass of the entire asteroid belt is 25 times less than that of the moons.
The Voyager 1 space probe reached this point in December 2004. This is the region where the heliosphere ends and interstellar space begins. This is the heliopause. In 2012, Voyager crossed this boundary and became the first human-made object to enter interstellar space. However, the message from Voyager reporting this event arrived on Earth almost a year later due to the vast distance. We’re so far away from home that even light takes longer than four years to travel this distance; if we used a conventional rocket, the journey would take 73,000 years. The reason we wanted to get here is because Proxima Centauri B has an Earth-like planet. It lies in the habitable zone of its host star, which means that liquid water could exist on the planet and life can form there. However, the star occasionally produces flares, and its brightness has increased almost 1,000 times in the past few years. During that time, it emitted so much radiation that, even if there were some forms of life on the planet, they probably no longer exist. This is trappist-1d. We’ve traveled 39 light years to reach a potentially habitable planet 39 light years from Earth. Its host star is a white dwarf, which is a cold star 10 times smaller and lighter than the Sun. It has seven planets orbiting it, but Trapist-1 is the most similar to Earth. It’s only 30 percent smaller and three times lighter than Earth, but it has a rocky surface and a temperature of 48 degrees Fahrenheit. It might have an atmosphere, mountains, seas, and oceans, which means it could be suitable for a human colony. Beetlejuice: It takes nearly 8.7 million years longer to travel here from Earth than a modern spacecraft. This star is so massive that our ship appears to be a grain of sand on a beach.
We must travel back in time to discover what happened to this star. It’s a cloud of multicolored space dust and debris that began to contract under its own weight as a nuclear reaction began in the core of the nebula and the star was born. At first, Beetlejuice was very massive and hot, but it didn’t expand and remained stable. Let’s take a look at its heart, where nuclear reactions produce a great deal of heat and energy. This energy produces the force that pushes on the walls of the star from the inside, causing it to expand. However, the star is extremely heavy, which is why gravity pushes on it from the outside. If these two forces are balanced, the star remains stable. However, as the star runs out of its fuels, helium and hydrogen, heavier elements in the core join the nuclear reaction, releasing more energy and heat than gravity can contain. A strong stream of matter that will be ejected from the explosion site won’t reach the solar system until 6 million years later. However, the solar wind will stop this flow, so we’re safe. It is likely to explode within the next ten thousand years, but some scientists say it won’t occur within the next hundred millennia. Getting back to the moment before Beetlejuice exploded, there is a more interesting scenario. Gravity may compress the massive core of the star with sufficient force to create a black hole. Black holes are the heaviest objects in the universe; even light cannot escape their gravitational pull. The Beetlejuice black hole will begin feeding on cosmic dust and whatever is left of the star. All this debris and light from other stars will get frozen near the event horizon of the growing black hole. For the first time ever, we’ll be able to watch the birth of this mysterious object.
However, Beetlejuice is actually too light to be a black hole. Over a million Earths can fit inside our sun. Twenty-five to 35 percent of suns consume their own planets, and a quarter of planetary systems orbiting stars like the sun had a chaotic past. The very thing that gives life can also take it away. All the planets in our solar system revolve around the Sun, and they do so in a relatively consistent manner. It’s likely that they’ve remained this way ever since they first appeared in the picture. This chaotic existence means that a solar system had many planets until the host’s son melted them away. Our solar system is perfectly arranged so that no planet’s gravity interferes with each other. Jupiter’s gravitational force is much stronger than Earth’s, which means that if Earth were to get close to Jupiter, we would become another moon for Jupiter. Jupiter is so large that if Earth were the size of a grape, Jupiter would be the size of a basket. Observing binary systems is the optimal method for studying this phenomenon. That’s just a scientific term for a system with two stars orbiting each other. Typically, the two stars were formed around the same time from the same gases and under the same conditions, so they should contain roughly the same elements. When you open your eyes in the morning, you’re greeted by sunlight that has traveled millions of miles. The closer we get to the sun, the hotter it gets, but the sun’s rays also contain certain chemicals that make them distinct. The study of these elements can reveal the history of a solar system in sufficient detail to determine whether it was disorderly or orderly.
Scientists studied 107 binary systems consisting of suns similar to ours by analyzing their light. Since each system contains two suns, they compared and contrasted them to determine the differences. They observed that stars with a thin outer layer had different elements than their companions. These elements are associated with rugged terrain on Earth, but they’re out there floating in space. The thinnest outer layer is particularly iron-rich compared to the other layers. Many stars are born as twins; in fact, the majority of Milky Way stars have a partner in a binary system. This makes our sun a bit of an outlier; however, there are theories that the sun may have lost its twin in the past; it’s approximately 184 light-years away and is designated hd186302. Perhaps this is our lucky star. Thousands of stars are born in a stellar nursery, which is made up of gas and dust that gradually collapses under its own weight. Our sun may have begun in such a way 4.6 billion years ago, and when they’re mature, they usually travel with a companion. Scientists estimate that up to 85 percent of all stars could be in binary pairs or have more companions, but over 50 percent are in dual pairs. Traces of it can be found in the Oort cloud, which is a vast cluster of comets, space rocks, and ice in the outer reaches of the sun’s gravitational pull.
Since these objects are far from the Sun’s gravitational pull, they are easily knocked out of their orbit and into open space. Flying through such a space is identical to flying through any random void of space. The reason why some of these light elements in space contain rock elements found on the surface of a planet is because the sun knocked them off their orbit and devoured them as they got closer. This also occurs when a star becomes too large for its position and begins devouring everything around it. Ice caps can melt in a matter of seconds and flood the coastal lands; even small islands in remote areas of the world will be submerged; and as it gets hotter, every snow-capped area will melt instantly and turn into desert-like climates; some places will burn; your everyday objects will melt on the spot; and Antarctica will melt from the heat as well as the volcanoes erupting across the globe. Earth will probably also be on the menu. If Earth moved only 900,000 miles closer to the sun, it would become uninhabitable. This may seem like a lot, but it’s only four times the distance between the Moon and Earth. Detecting the chemical composition of the sun’s rays in solar systems that are further away could help scientists find other Earth-like planets. Since the atmosphere around planet-eating stars changes its chemical composition, we can detect which solar systems have had a calm past. What would happen to us and our planet if it grew as large as the sun? The earth’s diameter is 8,000 miles. Crossing it is equivalent to driving back and forth across the United States three times.
If you don’t think that’s a big deal, consider how much gas it would cost to repeat this journey 305 more times. This is the diameter of the sun compared to the diameter of the earth. The sun is unimaginably large, so what will happen to us if we catch up with it? There are four possible outcomes, depending on what we mean by “size of the sun.” In scenario one, the Earth will become as large as the sun, but its mass will remain the same, creating a colossal planet with the mass of a tiny Earth. The greater a planet’s mass, the stronger its gravity, and vice versa. Such a lightweight planet would be incapable of attracting anything to itself. Gravity is responsible for holding everything from pebbles to entire continents. I’m sure you can guess what would happen without gravity: we’d all turn into dust particles, and the Earth would become a dust cloud. Jupiter, do you know which of its moons will survive and exact final vengeance on us? It’s too far away to notice any changes except for an increase in the mass of the center of the system, so Pluto’s orbit comes closer to our two-star system, and that’s it. The Earth and the Sun would have to accept that Pluto would be their only friend now that the protoplanetary disk that formed our solar system billions of years ago no longer exists, so no more planets can be formed in our solar system. What would life be like? Well, because of the increase in the Earth’s rotation time, nights and days are now longer, and the North and South Poles probably experience a significant temperature drop. Even on our current small planet, the North and South Poles receive little sunlight, so if the Earth’s size increased, the area of the poles receiving sunlight would decrease even further.
On the plus side, there’s a lot more space now, and there’s no more overpopulation because the planet’s size is centuries have passed, and many of us have left without ever meeting or learning about other people, and that’s if we can walk at all; our bones cannot support our weight with such a great gravity, and our hearts have to work twice as hard to keep us alive; the birds can’t fly anymore; nothing can; all the existing trees fall down, and the new ones grow very close to the ground like grass; how is our ecosystem doing if we don’t interact with other people? I also assume that it would be much darker than we’re used to. Imagine what would happen if the Earth grew to the size of the sun. We’d probably need an artificial sun, and the temperature differences on the planet’s surface would be enormous. If you’re surprised, you’ve probably underestimated the size of the sun; it’s nearly 110 times larger than the earth. Since the Earth has become four times as massive as the sun, it would have burned through its fuel faster than it could evolve. Depending on the mass of its core, the Earth either becomes a supernova or sheds its outer layers to form a planetary nebula. If it goes supernova, the sun that was so close to us survives, and all that’s left is our ex-Earth, a teeny tiny ball with a diameter of 12.5 miles. We’re a neutron star, which is a star made of degenerate neutron matter. It’s very dense and spins very quickly, so you’d better stay away from it. If the Earth becomes a nebula, the sun absorbs all the dust, the brightest light you’ve ever witnessed flashes, and our ex-Earth disappears.
It’s actually impossible for a rocky planet to be as large as the sun; only other stars can reach that size. However, why is the Earth so small compared to the other planets? Do they just keep growing, or do they reach a certain size? As planets become more massive, gravitational compression increases, and planets stop growing when their mass reaches approximately 1.7 times that of Jupiter or 540 times the mass of the earth. After that, adding more mass to a planet causes it to shrink because the compression becomes stronger; therefore, our thought experiment is impossible.
FAQ
What planet is in Beetlejuice?
Beetlejuice, sometimes written Betelgeuse, is a red supergiant star in the constellation Orion rather than a planet. It is among our galaxy’s biggest and brightest stars. Although Beetlejuice isn’t connected to any particular planet, it is a component of the Orion constellation, one of the most noticeable and easily identified in the night sky. Beetlejuice is a star that stands out for its reddish-orange hue and fluctuating brightness. Astronomers are interested in it because it is predicted to someday explode as a supernova, though when exactly this will happen is still unknown. In the night sky, it’s important to distinguish between stars and planets; Beetlejuice is a star, not a planetary body.
Is Betelgeuse going supernova 2023?
There was no solid scientific forecast or consensus that Betelgeuse would go supernova in 2023. The red supergiant star Betelgeuse resides in the constellation Orion. It has been fluctuating in brightness, with a substantial dimming in 2019. However, it is difficult to forecast when a supernova may occur. The precise timing of Betelgeuse’s supernova is yet unknown, but astronomers are keeping a watchful eye on it and other stars in case they exhibit any notable changes.
Is Beetlejuice a planet or a sun?
Often referred to as “Beetlejuice,” Betelgeuse is a crimson supergiant star that is neither a planet nor a sun. Betelgeuse, one of the biggest and brightest stars in the universe, is a star in the constellation Orion. Betelgeuse is one of the stars in the group of celestial bodies made mostly of hydrogen and helium, which combine nuclearly in their cores to produce heat and light. Stars are big enough to produce their own energy through nuclear fusion, in contrast to planets, which circle stars. Betelgeuse is distinguished by its characteristic reddish-orange hue and fluctuating luminosity. Though not the sun, which is the name usually given to the center star of our solar system, Betelgeuse is an important object in space that astronomers are interested in because of its size, its position in the stellar evolution, and the possibility of a supernova in the future.
Will Betelgeuse reach Earth?
As a far-off star in the constellation of Orion, Betelgeuse is not a direct threat to Earth. Even though Betelgeuse is a big red supergiant, it will take a very long time for it to explode like a supernova. Approximately 640 light-years separate Betelgeuse from Earth. The ensuing explosion, even in the event of a supernova, won’t directly affect Earth. Supernova explosions emit a tremendous quantity of light and energy, yet their impacts get smaller the farther away they occur. Astronomers predict that Betelgeuse’s supernova will be a stunning astronomical event to witness when it occurs, providing important insights into the life cycle of huge stars, even though the exact timing of the event is yet unknown. It is crucial to stress, though, that Earth is much beyond the physical reach of any potential supernova from Betelgeuse.
Does Betelgeuse still exist?
There is still betelgeuse. One of the brightest and most well-known stars in the night sky is Betelgeuse, a red supergiant star in the constellation Orion. Betelgeuse attracted the attention of skywatchers and astronomers in late 2019 and early 2020 when its brightness appeared to be decreasing, raising the possibility of an approaching supernova. But by the middle of 2020, Betelgeuse’s brightness started to increase again, reaching more normal levels. Betelgeuse and other stars naturally fluctuate in brightness; this is a regular aspect of their stellar behavior. Astronomers will be keeping a close eye on Betelgeuse, and the scientific community will be interested in any noteworthy changes that may occur.
Will Betelgeuse go black hole?
It is not anticipated that Betelgeuse will turn into a black hole. As a red supergiant, Betelgeuse is currently nearing the end of its star life cycle and is expected to have a supernova outburst in the future. A massive explosion known as a supernova will occur when Betelgeuse runs out of nuclear fuel and the core collapses due to gravity. Rather than becoming a black hole, the relics of this catastrophe are more likely to become a neutron star. Betelgeuse’s mass is thought to be between 10 and 20 times that of the Sun, which is less than what is needed for a planet to directly collide with a black hole. Although the precise moment of Betelgeuse’s supernova is yet unknown, the creation of a black hole is not anticipated. Astrophysics finds the evolution of big stars such as Betelgeuse to be fascinating, and the ultimate supernova event will provide important new information about stellar processes.
