Visible Universe
Visible Universe

How Big Is The Universe Compared To A Human?

Are you struggling to grasp the sheer scale of the cosmos? At COMPARE.EDU.VN, we break down the universe’s immensity in relatable terms, comparing it to the human scale, offering a fresh perspective on our place in the cosmos. Explore the vastness of space and discover how logarithmic scales and familiar analogies can make the universe feel a little less distant.

1. Understanding the Scale of the Universe: A Daunting Task

For most people, trying to understand how big the universe really is seems like an ant trying to understand the distance from New York to California. Human beings exist on the scale of meters, with the average human being a little less than two meters in height. Our typical experiences might take us three or four orders of magnitude away from that scale: down to millimeter scales or a little bit smaller, and up to scales of several kilometers. Beyond that, however, we have to stop thinking of the world in scales that we experience and get very abstract; it’s simply beyond what we’re familiar with on a day-to-day basis, and beyond what our senses are capable of perceiving and making sense of.

1.1 The Visible Universe: An Immense Expanse

The extent of the visible Universe now goes on for 46.1 billion light-years: the distance that light emitted at the instant of the Big Bang would be located from us today, after a 13.8 billion year journey. As time marches on, light that’s even farther away, that is still on its way to us, will eventually arrive: from slightly greater distances and with slightly greater redshifts. We see into the past when we look out to great distances because the light emitted from distant objects must traverse those great intergalactic distances at a finite speed: the speed of light.

1.2 The Microscopic World Within Us

It can feel overwhelming to go straight to such magnificently large scales that span tens of billions of light-years. If you were to examine your body under a microscope, you’d discover that you were largely composed of cells: biological units that bind together and move through your various systems to perform an invaluable series of life processes; all told, there are some 80-100 trillion cells inside a typical adult human body.

And yet, cells themselves — normally just tens to hundreds of microns in size — are themselves composed of smaller constituents: organelles, cytoplasm, along with various proteins, nucleic acids, and other simple and complex molecules. Molecules themselves are made out of atoms just 100 picometers across, while atoms are composed of point-like electrons that orbit nuclei that are only ~1 femtometer wide. Nuclei are made of protons and neutrons; each of those are made of point-like quarks and gluons, and while we know that electrons, quarks, and gluons are no bigger than about 10-19 meters, they could truly go all the way down to infinitesimally small scales.

2. Breaking Down the Numbers: From Atoms to Stars

There are many true, interesting, but difficult-to-comprehend facts that we could state about our constituent parts. For example:

  • Most of a human body’s mass is made of just the ~4 trillion cells that compose our musculoskeletal system, connective tissues, and internal organs. Another ~40 trillion cells are simply blood cells flowing through our body, and about ~50 trillion are bacterial cells — not even made by our own body — that live in our digestive tracts.
  • There are nearly 10^28 atoms in a human body, all told, and close to 10^29 subatomic particles that make each of us up. These numbers are huge: about 10-100 million times the total number of stars in the Universe.
  • And if you decided to fill the volume of an adult human being up entirely with, say, neutrons, you’d be able to fit more than 10^43 neutrons inside, with a total mass of around 20 trillion tonnes.

2.1 Building Up Scale: A Step-by-Step Approach

To a quark, a proton is understandable. To a proton or neutron, an atom takes up accessible scales. To an atom, a molecule is only a little bit larger. To a molecule, organelles aren’t so bad. To an organelle, a cell is a reasonable amount larger. To a cell, a bone or organ is within reach. And the human body is quite accessibly made up of those. To understand the scale of the Universe, we just have to build up a little bit at a time.

3. From Human to Earth: A Manageable Leap

One of the most convenient ways to begin is to go from the scale of a human to the scale of planet Earth. Although Earth is pretty big compared to a human, building up a little at a time doesn’t seem so bad. Human beings are capable of climbing mountains, and mountains can easily rise up several kilometers in elevation over sea level. If you rise up in a hot air balloon or an airplane, you can achieve heights of tens of kilometers. Aboard a space ship, you can escape to above Earth’s atmosphere, achieving altitudes of hundreds of kilometers, comparable to what one would see from the International Space Station.

3.1 The Overview Effect: Seeing Earth’s True Form

And as you move farther and farther from Earth, you get to see what it’s truly all about. It’s a spinning, nearly spherical ball about 13,000 kilometers in diameter. From only tens of kilometers up, you can start to see its curvature, and once you’re a few thousand kilometers away, you can take the full planet in one hemisphere at a time. Earth is extremely large compared to the scale of a human, but humans have ventured far enough away from planet Earth to obtain precisely this view, feeling a phenomenon known as the Overview Effect.

4. Earth to Solar System: Expanding Our Horizons

The Earth, however, is on the small side compared to many of the other bodies in our Solar System. Uranus and Neptune are each about four times the diameter of Earth, while Jupiter and Saturn are more like 10-11 times our planet’s diameter. The Sun — the largest object in our Solar System — is a staggering 1.4 million kilometers in diameter: some 109 times the diameter of Earth and capable of fitting more than one million Earths inside of it.

4.1 Orbits: The Scales of Planetary Motion

But the individual objects are easy to comprehend if you’re already the size of the Earth. And from the perspective of the Earth, it makes sense not only to look at the objects themselves, but the scales at which these objects move around one another: on the scales of planetary orbits. The Earth’s is the one we’re most familiar with: with a mean distance from the Sun of 150 million kilometers (or 93 million miles). But this distance, the Earth-Sun distance, is only a little more than 100 times the size of the Sun itself, which is only a little more than 100 times the size of the Earth itself. All of a sudden, by just going up a little bit: from on Earth to above Earth’s atmosphere and by looking at the other objects in our Solar System, we’ve gone from the scale of a ~1.5-2 meter human to a ~150 billion meter orbit around our Sun.

5. Solar System to Nearest Stars: A Giant Leap

Our Sun is just one of a great many stars in the Milky Way, so the next step up is from the scale of things in our Solar System (like Earth’s orbit) to the nearest stars. This is a huge jump, but one that we can comprehend if we now begin our starting point where our last endpoint left off: at the scale of Earth’s orbit.

5.1 The Oort Cloud: The Outer Limits of Our System

Other planets, of course, are farther away from the Sun than Earth is. Jupiter’s orbit is about 5 times the diameter of Earth’s; Saturn’s is 10 times as large; Uranus’s is 20 times as great; Neptune’s is 30 times as great. The Kuiper belt extends out to about double the extent of Neptune’s orbit, and while there are a smattering of other objects beyond that, you have to go out to around 1000 times Earth’s orbit before you reach the innermost portions of the Oort cloud. But the Oort cloud goes out for tens of thousands of times the Earth-Sun distance: perhaps out to even more than a full light-year. And then, once you start reaching distances of a few light-years, you finally reach it: the next nearest star to Earth, Proxima Centauri, located 4.2 light-years away.

5.2 Measuring Stellar Distances in Light-Years

Stars are separated by distances that are usually measured in light-years, and they add up fast. There are hundreds of stars within 25 light-years of us, and that number rises up to more than 10,000 stars if you draw a sphere just 100 light-years around Earth. At this scale, you start to notice that there are directions in space where there are more stars and other directions have fewer: you’re starting to see the structure of the Milky Way. In the direction of the galactic center, as well as throughout the plane of the Milky Way and particularly along its spiral arms, stars are denser and more numerous; away from them, less so.

6. Stars to Galaxies: Building Cosmic Structures

A galaxy is a collection of an enormous number of stars, but not an incomprehensibly large one. The Milky Way is a little over 100,000 light-years in diameter, which is to say that if a ~1.5-2 meter human being lives on a 13,000 kilometer-wide Earth, then that’s the same ratio as the distance to the inner Oort cloud to the size of the Milky Way.

6.1 Analogies for Galactic Scale

Humans-to-Earth is the same as the size of Earth to the distance to the inner Oort cloud is the same as the distance to the inner Oort cloud is to the size of the Milky Way. Stars are tiny compared to the distances between them. If the Sun were a grapefruit in Seattle, WA, then the next nearest star would be a grapefruit in New York.

7. Galaxies to the Observable Universe: The Grandest Scale

Galaxies are not tiny compared to the distances between them. If the Milky Way were a grapefruit in Seattle, WA, then Andromeda — the Local Group’s largest galaxy located 2.5 million light-years away — would be a grapefruit in the same room, only about 10 feet (3 meters) away. In fact, the Virgo Supercluster, spanning perhaps one hundred million light-years, contains thousands upon thousands of large galaxies, and that would be like having thousands of grapefruits clustered and clumped together in groups over the span of about a single city block.

7.1 The Large-Scale Structure of the Universe

The large-scale structure of the Universe is kind of like that: there are hundreds of billions of grapefruits — and tens of trillions of, say, oranges, mandarins, and kumquats that are smaller versions of galaxies — distributed across just under 500 such “city blocks” in all directions in all three dimensions, with ours, containing the Virgo Cluster, located at the center. If 100 million light-years is well within our Local Supercluster, then it’s only some 460 times that distance to the edge of the observable Universe.

8. Comprehending the Incomprehensible: From Human to Universe

From the scale of a human to the scale of the observable Universe seems incredibly daunting. Humans are a couple of meters in scale; the Universe that we can see extends for some 46 billion light-years in all directions. That means the observable Universe — in terms of diameter — is nearly a full 27 orders of magnitude, or a factor of one octillion (1,000,000,000,000,000,000,000,000,000) larger than a human being. It’s easy to see why that’s so wildly incomprehensible.

8.1 Two Tricks for Understanding Scale

That’s why we use two tricks at once:

  1. We don’t go straight in one magnificent leap from one accessible scale to the largest or smallest scales, but rather we go in as many reasonable steps as it takes so that no two “steps” are too far apart.
  2. And we don’t necessarily look at everything on the same objective scale, but rather we change our perspective with each successive step.

8.2 The Logarithmic Perspective

One of the more intuitive ways to take both of these steps, together, is instead of thinking in conventional distances, to think of distances from a logarithmic point of view. In fact, a logarithmic map of the Universe, like the one shown below, can truly capture the grandeur of the Universe on a variety of scales all at once.

9. Our Place in the Universe: Significance Beyond Scale

The way to conceive of scales as big as the Universe is not from the perspective of a human, but rather from the perspective of something more relevant to the Universe itself. The Universe is big, but it’s only a few hundred thousand times as big as the Milky Way galaxy. The Milky Way galaxy is big, but it’s only a few tens of thousands of times as big as the distance between any two typical stars. The distance between any two stars is pretty big, but it’s only a few hundred thousand times as big as the Earth-Sun distance. And the Earth-Sun distance is only ~10,000 times as big as the Earth, which is, at last, accessibly-sized to human beings.

9.1 Cosmic Neighbors: A Sense of Belonging

If you insist on taking the leap from ourselves up to the size of the observable Universe, it’s easy to feel insignificant. But we are a part of many significant things that fit better on larger scales; we can view ourselves as creatures of Earth, members of the Solar System, a component of the Milky Way, and inhabitants of this Universe. This isn’t an inconceivably large place; rather, it’s the full extent of our home as best as we know it, and the nearby and distant objects beyond our own planet are our cosmic neighbors and relatives. Although they might seem inconceivably far away, from the perspective of the Universe, anything we can see is really just cosmically right next door.

10. Frequently Asked Questions (FAQ)

Here are some frequently asked questions about the size of the universe compared to a human:

  1. How much bigger is the universe than a human?

    The observable universe is approximately 27 orders of magnitude larger than a human, or one octillion times bigger.

  2. What is the size of the observable universe?

    The observable universe has a diameter of about 93 billion light-years.

  3. How many stars are in the universe?

    There are estimated to be around 10^24 stars in the observable universe.

  4. What is a light-year?

    A light-year is the distance light travels in one year, approximately 9.461 x 10^12 kilometers.

  5. Why is it difficult to comprehend the size of the universe?

    The scales involved are so vastly different from our everyday experiences that it’s challenging for the human brain to grasp.

  6. What is the largest structure in the universe?

    The largest known structure is the Hercules-Corona Borealis Great Wall, a galaxy filament about 10 billion light-years long.

  7. How does the size of Earth compare to the Sun?

    The Sun is about 109 times the diameter of Earth and can fit over a million Earths inside it.

  8. What is the Milky Way?

    The Milky Way is our galaxy, a spiral galaxy containing billions of stars, including our Sun.

  9. How far is the nearest star to our Sun?

    The nearest star to our Sun is Proxima Centauri, located about 4.2 light-years away.

  10. How do astronomers measure distances in space?

    Astronomers use various methods, including parallax, standard candles (like supernovae), and redshift measurements.

Conclusion: A New Perspective on Our Place in the Cosmos

Understanding the immense scale of the universe is a journey, not a destination. By breaking down the cosmos into manageable steps and shifting our perspective, we can begin to grasp the true extent of our cosmic home.

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