Category: sun

Ask Ethan: Will The Earth Eventually Be Swallowed By The Sun?

“When the Sun eventually goes Red Giant, will the Earth simply be orbiting within the outer envelope of the sun, or will something more interesting happen?”

In 2008, a now-famous astronomy paper was published that purported to determine the fate of the Earth as the Sun swelled to become a red giant. In particular, it claimed that not only would Mercury and Venus definitely be engulfed, but that the Earth would be, too. Sure, the Sun loses mass, which causes the planets to spiral outward, but it also grows in size, which leads to both drag forces on the orbiting planets as well as tidal forces that can sap a planet’s orbital angular momentum. The authors concluded that Earth’s orbit would need to presently be about 15% larger in order for it to have a chance of surviving. But there are other important factors at play, and they legitimately could change the outcome. 

The smart money might still be on the Earth getting swallowed, but it’s far from a settled issue. Come learn where we are in our understanding of how the Solar System will evolve in the far future!

This Multi-Trillion Dollar Disaster Is Coming, And Solar Astronomy Is Our Prime Defense

“Although the largest solar flares are rare, they do occur with some regularity. Some of them create coronal mass ejections; some coronal mass ejections head directly towards Earth; some of the ones that do head towards Earth have exactly the right properties to create spectacular aurorae and potentially catastrophic geomagnetic storms. Only now, with this new generation of solar astronomy tools, are we finally in position to scientifically prepare for the inevitable disaster.

For decades, we’ve avoided the ruination of our modern infrastructure through sheer luck alone. A Carrington-level event, if it were to strike us unawares, would certainly cause trillions of dollars worth of damage worldwide. With the advent of these new heliophysics-focused observatories, led by the NSF’s Daniel K. Inouye Solar Telescope, we’ll finally have the opportunity to know when “the big one” is coming.”

In 1859, solar astronomer Richard Carrington was observing the Sun, when a “white light flare” danced around a massive sunspot for around five minutes before disappearing. 18 hours later, the largest geomagnetic storm in recorded history struck Earth. If such an event were to occur today, the induced currents it would create could cause trillions of dollars worth of damage.

But there’s a scientific way to know if one is coming, not just minutes in advance but from the moment the Sun releases a coronal mass ejection: through solar astronomy. In particular, the National Science Foundation’s new Inouye Solar Telescope, whose first light image has delighted the public across the world, will provide our first line of defense against this Sun-driven catastrophe, as well as our first early warning signal.

As spectacular as our first images of the Sun with this new observatory are, there’s a science goal that’s relevant to us all. This is why we study the Sun as we do.

This Is The One Way The Moon Outshines Our Sun

“Unlike the Sun, the Moon’s surface is made of mostly heavier elements, while the Sun is mostly hydrogen and helium. When cosmic rays (high-energy particles) from throughout the Universe collide with heavy atoms, nuclear recoil causes gamma-ray emission. With no atmosphere or magnetic field, and a lithosphere rich in heavy elements, cosmic rays produce gamma-rays upon impacting the Moon.”

When you view the Moon with your eyes, you’re not seeing it shine so brightly because it’s emitting its own light. Rather, it’s reflecting sunlight on its illuminated phase and reflecting light emitted from Earth (known as “Earthshine”) on the darkened portion. If you look at the Moon in many different wavelengths, from radio to infrared to ultraviolet to X-ray energies, you’ll find that the Sun is much brighter, and the Moon primarily emits light due to reflection.

But in gamma-rays, that entire story changes. The Sun emits virtually no high-energy gamma-rays, with only minor bursts during solar flared. The Moon, on the other hand, emits high-energy gamma-rays constantly; for almost 30 years we know that it outshines the Sun in this particular wavelength range.

It might sound puzzling to you, but there’s a good physics reason for this, and a fun little science fact that everyone should appreciate. Get the story today!

Astronomers Debate: How Many Habitable Planets Does Each Sun-Like Star Have?

“We know that there are between 200 billion and 400 billion stars in the Milky Way galaxy. About 20% of those stars are Sun-like, for about 40-to-80 billion Sun-like stars in our galaxy. There are very likely billions of Earth-sized worlds orbiting those stars with the potential for the right conditions to have liquid water on their surfaces and being otherwise Earth-like, but whether that’s 1 or 2 billion or 50 or 100 billion is still unknown. Future planet-finding and exploring missions will need better answers than we presently have today, and that’s all the more reason to keep looking with every tool in our arsenal.”

Most of the time, in science, the quality of our data drives the size of our uncertainties. When we have very little data and it’s only of poor quality, our uncertainties tend to be large; when we have lots of very good data, our uncertainties shrink. NASA’s Kepler mission has provided astronomers with an unprecedented suite of data on exoplanets, revealing thousands of new worlds beyond our Solar System. And yet, despite all it’s found, if you ask the simple question of “how many Earth-like planets orbit a typical Sun-like star,” answers disagree by a factor of 100: from about 1% of stars have them to there’s between 1 and 2 for each and every such star.

What’s the real story? Where do these uncertainties arise, and are they larger than they need to be? Come get the full story (and watch David Kipping’s video at the end) and find out!

This Is Why We Don’t Shoot Earth’s Garbage Into The Sun

“Considering that the United States alone is storing about 60,000 tons of high-level nuclear waste, it would take approximately 8,600 Soyuz rockets to remove this waste from the Earth. Even if we could reduce the launch failure rate to an unprecedented 0.1%, it would cost approximately a trillion dollars and, with an estimated 9 launch failures to look forward to, would lead to over 60,000 pounds of hazardous waste being randomly redistributed across the Earth.

Unless we’re willing to pay an unprecedented cost and accept the near-certainty of catastrophic environmental pollution, we have to leave the idea of shooting our garbage into the Sun to the realm of science fiction and future hopeful technologies like space elevators. It’s undeniable that we’ve made quite the mess on planet Earth. Now, it’s up to us to figure out our own way out of it.”

As human beings continue to lead the technologically advanced lives we’re presently leading, we’re also producing waste of many different types. Biohazards, dangerous chemicals, nuclear waste and other pollutants must be kept out of drinking water, agricultural regions, the oceans, atmosphere, and away from populated areas. You might wonder why, now that we’re well into the space age, we haven’t considered shooting Earth’s most difficult-to-deal-with garbage into the Sun?

Well, we have considered it, and there are good reasons not to do it. If you’ve ever wondered why, you’ll really enjoy this read.

This Is What Will Happen To Our Sun After It Dies

“During the red giant phase, Mercury and Venus will certainly be engulfed by the Sun, while Earth may or may not, depending on certain processes that have yet to be fully worked out. The icy worlds beyond Neptune will likely melt and sublimate, and are unlikely to survive the death of our star.

Once the Sun’s outer layers are returned to the interstellar medium, all that remains will be a few charred corpses of worlds orbiting the white dwarf remnant of our Sun. The core, largely composed of carbon and oxygen, will total about 50% the mass of our present Sun, but will only be approximately the physical size of Earth.”

Looking forward in time, the death of our Sun is easy to envision, as we’ve seen Sun-like stars in their dying phases and immediately afterwards plenty of times. But what happens after that, in the far future? Will our Sun’s corpse remain a white dwarf forever? Will it simply cool down, radiating heat away? Or will something exciting happen?

Maybe we’ll get ejected from the galaxy. Maybe we’ll get devoured by a black hole. Maybe we’ll merge with another object, or experience an interaction that forever changes us from what we were. Maybe we’ll even experience a cataclysm that destroys our stellar corpse entirely!

Although the possibilities are fascinating, there’s an overwhelming statistical likelihood that points to one particular outcome. What is it? Find out today!

Earth: Hi sun!

Sun: …

Earth: …

Sun: Dad?

This Is How The Sun Moves In The Sky Throughout The Year

“It’s easy to see that the topmost point corresponds to the summer solstice, while the lowest point corresponds to the winter solstice, but there is no special astronomical significance to the “crossing-point” in the Sun’s analemma as seen from Earth. Occurring approximately on April 14th and August 30th, those dates are only determined by the way our seasons, determined by axial tilt, align with our planet’s orbit around the Sun.

If our perihelion and aphelion were aligned with the equinoxes, rather than the solstices, we’d have a teardrop-shaped analemma, rather than a figure-8, which is how the Sun appears from Mars! The analemma is the beautiful, natural shape traced out by the Sun over time, creating a figure-8 as both our orbit and axial tilt dictate. Enjoy the Sun’s motion through our skies, as its unique cosmic pirouette is due to our planet’s one-of-a-kind motion through space!”

You might notice that the Sun is changing its position in the sky, while sunset and sunrise times also change. But did you know that you’d get this bizarre, pinched, figure-8-like shape if you took a picture of the Sun every day throughout the year at 24-hour intervals? It’s true! The shape is known as Earth’s analemma, and it’s determined by a variety of factors that you must consider all of in order to get the explanation right. 

Come learn how (and why) the Sun moves the way it does throughout a year as seen by every location on Earth, including yours!

-BuT wHaT dOeS iT hAvE tO dO wItH sCiEnCe?


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