From EarthSky: “What is interstellar space?” An Old But Important Story


From EarthSky

October 10, 2020

In this infrared image from NASA’s Spitzer Space Telescope, winds flowing out from a fast-moving star (Zeta Ophiuchi) are making ripples in the dust in interstellar space. Credit: NASA.

NASA/Spitzer Infrared telescope no longer in service. Launched in 2003 and retired on 30 January 2020. Credit: NASA

Interstellar space – the space between the stars – isn’t just empty space. There’s a lot of “stuff” out there, including hydrogen (70%) and helium (28%), formed in the Big Bang that set our universe into motion. The other 2% of “stuff” in interstellar space is heavier gases and dust, consisting of the other elements made inside stars and spewed into space by supernovae. The material in interstellar space is very spread out. It’s denser in some places than in others, but a typical density is about one atom per cubic centimeter. Still, even the most dense regions of interstellar space count as vacuum, compared with our earthly air.

Our sun controls the conditions around our solar system, but outside of that is interstellar space and all that it contains.

Astronomers call this space between the stars the interstellar medium.

SDSS map is shown as a rainbow of colors in the observable Universe. Credit Anand Raichor (EPFL) Ashley Ross (Ohio State) and SDSS Collaboration.

Milky Way Galaxy from Sun to Interstellar Space beyond the Oort Cloud. Credit: NASA/ JPL-Caltech.

Why is interstellar space important?

The interstellar medium is where stars are made. Without it, we wouldn’t exist. If there weren’t thick and thin spots that condensed into thicker patches that eventually became stars, the whole universe would just be a cloud of boring, cold, lifeless gas.

The thick parts of the interstellar medium are called molecular clouds – often referred to as stellar nurseries – the places where stars are born. The first stars didn’t have planets because there weren’t any materials in interstellar space beyond hydrogen and helium. But, over the billions of years of our universe’s history, that has changed.

It changed because stars themselves make increasingly more complex elements in their interiors. When the most massive stars grow old and die, they explode as supernovae, releasing their elements into interstellar space. Thus it has become possible for stars to form with planets and for at least one planet we know of, Earth, to harbor living things.

Given the contents of interstellar space, and process by which stars and planets are born, it seems highly likely that other planets have living things, too.

This intriguing view of spectacular stellar nursery IC 2944 was released to celebrate a milestone: 15 years of ESO’s Very Large Telescope. This image also shows a group of thick clouds of dust – known as the Thackeray globules – silhouetted against the pale pink glowing gas of the nebula. Credit: ESO.

ESO VLT at Cerro Paranal in the Atacama Desert, •ANTU (UT1; The Sun ),
•KUEYEN (UT2; The Moon ),
•MELIPAL (UT3; The Southern Cross ), and
•YEPUN (UT4; Venus – as evening star).
elevation 2,635 m (8,645 ft) from above Credit J.L. Dauvergne & G. Hüdepohl atacama photo.

Our solar system, and spacecraft, in interstellar space

The sun is our local star. It’s about 870,000 miles (1.4 million km) across, approximately 100 times wider in diameter than our planet Earth. It would take more than 965,000 Earths to fill up the volume of the sun. Earth is one of the smaller planets in our solar system.

A stream of charged particles emanates from the upper layers of the sun’s atmosphere; this stream of particles is known as the solar wind. The sun – and its solar wind – create a kind of cavity that envelopes our entire solar system, known as the heliosphere. The heliosphere is like a balloon, with our sun and planets inside the balloon. Outside the heliosphere is interstellar space.

Neptune, the farthest of our solar system’s major planets, is 30 times the distance from the sun as Earth. We call the distance from Earth to the sun an astronomical unit (AU), so Neptune is at a distance of 30 AU.

The edge of the heliosphere is four times as far, at about 120 AU.

The heliosphere is moving through the space of our Milky Way galaxy. As it moves, the part of the heliosphere that faces the center of our galaxy receives more pressure than the side that faces away, so the heliosphere is stretched out into a teardrop shape.

Illustration of the positions of the Voyager 1 and Voyager 2 spacecraft – the farthest spacecraft from Earth – now both outside of the heliosphere, in interstellar space. Voyager 1 crossed the heliopause, or the edge of the heliosphere, in August 2012. Heading in a different direction, Voyager 2 crossed another part of the heliopause in November 2018. The Voyagers revealed that the size of the heliosphere changes. It seems to “breathe” in a way related to the level of the sun’s activity, getting bigger when the sun is active, and shrinking when it’s quiet. Heliosphere-heliopause showing positions of Voyager spacecraft. Credit: NASA.

Presumably, every star creates its own bubble around itself. At the edges of all these billions of “heliospheres,” stars leak particles and electromagnetic radiation into space, further feeding the interstellar medium.

Once you have traveled past the inner edge of the heliosphere, there is a region called the termination shock that is like white-water rapids in a stream.

Finally it smooths out and you enter the heliopause, an area where the internal pressure of the sun’s effect balances with the outside pressure of the interstellar medium. It is very still, where you finally enter interstellar space itself.

About that “vacuum” of space …

When we talk about space, we often think of vacuum where there is absolutely nothing for us to breathe. Earth’s atmosphere is quite thick at sea level. It extends well above the International Space Station (ISS), but it is so thin that after a few hundred kilometers, it’s almost as if it isn’t there. Earth’s atmosphere may finally end around 6,700 miles (10,800 km) above Earth’s surface, or higher, depending on whom you ask.

On Earth at sea level, a cubic centimeter of air has 30,000,000,000,000,000,000 molecules in it, or we could say 3 with 19 zeros after it, but for convenience, we write it as 3 times 10^19. So in a volume just a little bit smaller than a normal die, there is an unfathomable amount of molecules.

At Mount Everest’s peak there are is a bit more than 10^18 molecules in the same volume, and, at the altitude of ISS (~350 km or a little over 200 miles up), there are only 1 million (10^6) molecules per cubic centimeter – and the same for the thin atmosphere of the moon.

In comparison, interstellar space only has about 1 atom per cubic centimeter on average, although this number varies from 100,000 to as low as 0.01 depending on if you’re in a molecular cloud or in the space in between the clouds. Either way it’s about as close to an absolute vacuum as you can get (not counting intergalactic space where the number is even lower …).

The layers of Earth’s atmosphere. Graphic via NOAA.

See the full article here .

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Deborah Byrd created the EarthSky radio series in 1991 and founded EarthSky.orgin 1994. Today, she serves as Editor-in-Chief of this website. She has won a galaxy of awards from the broadcasting and science communities, including having an asteroid named 3505 Byrd in her honor. A science communicator and educator since 1976, Byrd believes in science as a force for good in the world and a vital tool for the 21st century. “Being an EarthSky editor is like hosting a big global party for cool nature-lovers,” she says.