The Space Between

Earth rising over the Moon's horizon, as captured from space during the Apollo 8 mission.

Space captivates me in a way few other things can. I’ll happily fritter away a Sunday learning everything I can about a new cosmic-related subject. Absorbing mind-breaking facts, agreed on by most of Earth’s brightest astrophysicists, that feel like fiction to a mind accustomed to things here on Earth. I always leave wanting to know more.

  • Like, how can a teaspoon (5 mg) of neutronium, the hypothetical substance made purely of neutrons that we believe is inside of every neutron star, weight 5.5 billion (5,500,000,000) metric tons?1
  • And how can a red dwarf, the smallest possible star, live for trillions of years2 when we believe the universe itself is only 13.8 billion (13,800,000,000) years old?3
  • Or how does the Sun convert 600 million (600,000,000) tons of hydrogen into 596 million (596,000,000) tons of helium every second?4

See what I mean about mind-warping? The science of space takes the numbers and measurements we are used to in everyday life and blows them up in spectacular fashion.

Earth rising over the Moon's horizon, as captured from space during the Apollo 8 mission.
Earthrise, taken on December 24, 1968, by Apollo 8 astronaut William Anders.
icon of an image NASA / Public Domain via Wikimedia Commons.

The distance between objects in space is one of those mind-bending things. It requires time to think about and consider before you can put it into perspective. The kilometer is the biggest unit of measurement, distance wise, in my day-to-day life. Low on groceries? The market is about 5 km away. Visiting my sister? That’s about 120 km. Even a flight from Toronto to Japan is just over 10,000 km, so when it comes to life on Earth, I don’t need anything much bigger than that to define distances.

Illustration of the Earth and Moon in space, showing the Moon's orbit around Earth with the distance between them labelled at 360,000 km.
Earth and the Moon.

Now let’s take a look at our closest cosmic neighbor. The Moon’s orbit is elliptical, so the distance between us isn’t always the same, but at its closest it’s about 360,000 km5 from us. That’s hundreds of thousands of kilometers from us! The Earth’s circumference at the equator, the longest possible journey around our planet, is just over 40,000 km, 1/9th the distance. If we had a highway between us and drove it at 120 km/h, it would take about 125 days6 of non-stop driving to get there. That’s a hell of a long way and this is the closest thing to us out there.

But hundreds of thousands is still a number we are used to seeing, right? If I told you I had $360,000 (I don’t), you would be happy for me (I assume), but you wouldn’t be in awe. It falls in the realm of numbers we come across in our Earth-shackled lives. So let’s go a little farther out.

When we look at the planets closest to us, things really start to get interesting. Venus, our sister planet,7 comes within 41,000,000 km8 from us. MILLIONS! We are a bit beyond comparing to car rides here because a drive to Venus would take about 39 years.9 I hope you brought a snack! It gets even more intense with Mars. The red planet’s closest approach to Earth is about 56,000,000 km.10 When NASA delivered its most recent Mars rover, Perseverance, the journey took more than 29 weeks, with the spacecraft hurtling through space at nearly 40,000 km/h.11 The trip isn’t a straight line and is significantly longer than 56,000,000 km (because space) but you get the idea. Getting anywhere off-planet, even our cosmic backyard, is really hard and takes a lot of time.

Illustration of Venus, Earth, and Mars in space, showing their closest distance (relative to Earth) with labeled measurements: 41,000,000 km between Venus and Earth, and 56,000,000 km between Earth and Mars.
Venus, Earth, and Mars.
Illustration of a yeti (head and shoulders only) in front of a flower pattern.
YETI SIDEBAR
Interested in why Perseverance’s trip to Mars was significantly longer than 56,000,000 km? To get to Mars, we follow the Hohmann transfer orbit, “an orbital maneuver used to transfer a spacecraft between two orbits of different altitudes around a central body.”12 The rover, launched on an Atlas V rocket into a Mars-bound trajectory, actually travelled a total of 471,000,000 km13 through space before reaching the red planet.🚀

Astronomical Unit14 (AU)

Comparing distances to Earth is a bit tricky because objects in our solar system are at the whims of the Sun, flinging us around her in gravity-powered orbits. Moving forward, let’s use old Sol as our starting point. The average distance between the Sun and Earth is about 149,600,000 km, a distance deemed important enough to get its very own unit of measurement, the astronomical unit (AU).15 Just under 150 million km. At this distance the Sun’s rays, travelling at the speed of light,16 take over 8 minutes to get to us. If our sun were to disappear all of a sudden, we would have no idea for 8 blissful minutes. I know what I’m doing 8 times.17

Average distance from the Sun (AU)Average distance from the Sun (km)
Mercury0.3957,910,000
Venus0.72108,200,000
Earth1.00149,600,000
Mars1.52227,900,000
Vesta2.36352,000,000
Ceres2.77414,000,000
Illustration of the inner solar system with their respective average distances from the sun in astronomical units (AU). Showing the Sun, Mercury (0.39 AU), Venus (0.72 AU), Earth (1 AU), Mars (1.52 AU), Vesta (2.36 AU), and Ceres (2.77 AU).
The inner solar system. The rocky planets reside between the Sun and the Asteroid Belt, a region of space measuring 2,2 AU (329 million km).

Our solar system has 98 planets,18 4 small rocky ones (inner solar system) and 4 big gassy/icy ones (outer solar system), separated by a conveniently-located belt of asteroids (brilliantly) named the Asteroid Belt. Neptune, the farthest planet from the Sun, is over 30 AU away but Mars, the farthest rocky planet, is only about 1.5 AU. So although the planets stack up even at 4-4 on the inner/outer solar system planetary counter, the latter is significantly bigger in terms of actual space occupied. Which I guess makes sense. They are called the gas and ice giants. They would need some room.

Six of our eight planets, including the two giants, sit within 10 AU of the Sun. But reaching Uranus means going another 10 AU and Neptune is another 10 beyond that. These last two planets are really far from us. Only one spacecraft, Voyager 2,19 has ever visited them. At those distances, sending large scientific instruments becomes a serious challenge, both technically and financially.

Illustration of the outer solar system showing planets and celestial objects with their average distances from the Sun in astronomical units (AU). Featured are Jupiter (5.20 AU), Saturn (9.59 AU), Uranus (19.19 AU), Neptune (30.07 AU), Pluto (39.48 AU), Haumea (42.11 AU), and the Kuiper Belt (30-50 AU). The background is a starry space with orbital paths indicated.
Part of the outer solar system. The gas and ice giants reside between the Asteroid Belt and the Kuiper Belt, a region of space measuring over 27 AU (6.7 billion km).
Average distance from the Sun (AU)Average distance from the Sun (km)
Jupiter5.20777,900,927
Saturn9.591,434,643,580
Uranus19.192,870,783,139
Neptune30.074,498,407,972
Pluto39.485,906,123,935
Haumea43.116,449,164,206

Anything in our solar system beyond Neptune is referred to as a trans-Neptunian object, or TNO. These are usually sorted into three groups: Kuiper Belt objects, Scattered Disc objects, and the far more distant Oort Cloud objects.

The Kuiper Belt (pronounced Ky-per), home to Pluto and about half a dozen other dwarf planets, is a vast ring of icy objects beyond Neptune. It’s similar to the Asteroid Belt, but stretches over 20 times farther and contains 20 to 200 times more mass.20 It is a relatively flat, disk-like region sitting on the same general plane as the planets, called the ecliptic plane. Near the end of the Kuiper Belt, the Sun’s gravitational pull has weakened enough that objects can be flung into eccentric, highly-inclined orbits due to Neptune’s big assmass. This region of space, known as the Scattered Disk, begins somewhere inside of the Kuiper Belt and goes on well past the 100 AU mark. Eris, the second-largest known dwarf planet in our solar system, is a bit smaller than Pluto, but way farther out, sitting at 67.86 AU from the Sun. That’s over 10 billion (10,000,000,000) kilometers. Light from the Sun takes 9 hours21 just to get there, and even then, our solar system keeps going.

Illustration of a yeti (head and shoulders only) in front of a flower pattern.
YETI SIDEBAR

How bright do you think the sun is at this distance?

A star’s brightness (solar irradiance) decreases with the square of the distance from the Sun.22 It’s measured in Watts / meter2

  • At 1 AU (like on Earth), it is 1361 W/m2.
  • At 2 AU, it is 340 W/m2.

So, \( I = \frac{1361}{(67.86)^2} \approx 0.296 \, \text{W/m}^2 \)

At Eris, sunlight has an intensity of ~0.296 watts per square meter, which is:

  • About 0.022% of what we get on Earth.23☀️
  • Still 295 times brighter than full moonlight on Earth (~0.001 W/m2).2425🌙
  • Bright enough to cast shadows and potentially require UV protection if looking near the Sun in space.🕶️

Voyager 1, launched by NASA in 1977 to explore the outer solar system, reached 167.34 AU in February 2025,26 which is about 25 billion kilometers. It is the most distant human-made object in space yet despite nearly 50 years of travel, it has covered only a tiny fraction of the distance to the nearest star beyond our Sun, which is an astonishing 268,000 AU away.

Science fiction has delivered a ton of fantastic stories about space travel and voyages to alien planets outside of our solar system, but making any of them a reality will be incredibly difficult, and maybe even impossible, simply due to the distances involved. That’s why some of the best stories include time dilation or other cool science quirks. With our current technology, we can’t exit our solar system in one person’s lifetime. Or even 10 people’s lifetimes. The distance is just too great.

NASA engineers in cleanroom suits install the golden record on the Voyager 1 spacecraft before its launch.
Gold plated record being added to Voyager 1.
icon of an image NASA / Public Domain via Wikimedia Commons.
An illustration of the Kuiper Belt, Scattered Disc, and Oort Cloud surrounding the Sun, with orbital paths of comets and celestial bodies depicted in a cosmic setting.
An illustration of the sun (inner yellow dot), Kuiper Belt (white donut), Scattered Disc (orange dashed lines), and Oort Cloud (outer sphere).

Astronomers believe the Scattered Disc to be the spawn point of most short-period comets,27 big dirty snowballs28 zipping around the Sun, with an orbital period under 200 years. Up to and over 100 AU from us, these objects are far but not as far as the Oort Cloud, the hypothetical home of long-range comets.29 Although only theorized, because we can’t actually see it, we believe there is a cloud of icy planetesimals that surrounds the Sun at a distance of 2,000 to 200,000 AU.

200,000 AU is just shy of 30 trillion (30,000,000,000,000) km. That number is so massive, it’s hard to even wrap your head around it. But let’s try anyway. Ever hear the “how many seconds are in a million compared to a billion” fact? I’ve seen it a few times in stories attempting to put billionaires’ money into perspective. Basically, if a person got 1$ every second, they would be a millionaire in under 12 days, but it would take almost 32 years to become a billionaire. Pretty big difference, right? Well, it would take over 950,000 years to hit 30 trillion.30🤯 Astronomical!!

Light-year (ly)

Proxima Centauri, one of the three stars in the Alpha Centauri star system, is the closest star to the Sun and is about 268,000 AU31 from us. Even using astronomical units, these numbers are starting to get big again so it’s time for a new unit of measurement, the light-year (ly). Simple enough to remember, it’s the distance light travels in one year. 1 ly is 63,241 AU so Próxima Centauri is 4.24 ly from the Sun.

The farther a star is, the further back in time we’re seeing it. When we look in the night sky and spot the Alpha Centauri system, we’re seeing it as it was over 4 years ago. If someone is on Próxima Centauri right now looking this way, they’re seeing me mid-Covid outbreak and I can’t even explain to them why I’ve gained 30 lbs and keep making so much bread.

Radar-style map showing the celestial bodies within 9 ly from the Sun including Alpha Centauri, Barnard's Star, Sirius, and others in light-year distance rings.
A radar map of the distances (▬) and positions (◆) marked of all known stellar bodies or systems within 9 light years (ly) of the Sun.
icon of an image Illustration by Nsae Comp. Via Wikimedia Commons. This image is licensed under the Creative Commons Attribution-Share Alike 4.0 International license.

Unless stars are in a system together, they usually have a lot of space between each other. So much so that when the Milky Way collides with the Andromeda galaxy in 4 to 5 billion years, astronomers believe the odds of any two stars actually hitting each other are extremely low.32 A cloud with billions of stars crashing into another cloud with billions of stars and none will actually hit each other? Seems implausible at first but only because our minds can’t actually visualize that much space. Our sun’s diameter is about 1,390,000 km (1.39 × 106 km) but the distance between Proxima Centauri and us is about 4.2 light-years (4.01 × 1013 km), which is approximately 29 million times bigger.33 You can fit a whole lot of other suns in there.

The Parker Solar Probe, a cool little probe NASA launched in 2018 to make observations on the Sun’s corona, is the current title-holder for fastest man-made object in space. It reaches speeds of 690,000 km/hour34 and it would still take over 6,600 years35 to reach Proxima Centauri, the star closest to our sun. A craft travelling almost 700,000 km/hour would still need over six and a half millennia to reach the closest star to us? I love trying to find relative ways like this to consider cosmic distances. It paints a picture in my brain.

Illustration of a yeti (head and shoulders only) in front of a flower pattern.
YETI SIDEBAR
The Parker Solar Probe is in my top-3 space things of the last decade. Assisted multiple times by Venus’ gravity, this little guy is zipping through space at incredible speeds. On Christmas Eve 2024, it made the closest approach ever to the Sun by a man-made object, passing within 6.1 million km from the surface, touching the Sun’s corona (atmosphere). The probe’s heat shield reached temperatures of 1,000° Celsius.36 Muy muy caliente!️‍🔥

Closest Stars to Us37

An illustration of the Alpha Centauri triple star system. 2 bigger yellow sun-like stars and 1 smaller red star on a background of starry space.

Alpha Centauri

A triple star system including binary sun-like stars and a red dwarf, they are between 4.24 ly and 4.35 ly from the Sun.

An illustration of Barnard's Star. 1 smaller red star on a background of starry space.

Barnard’s Star

A small red dwarf star in the constellation of Ophiuchus, it is 5.96 ly from the Sun.

An illustration of Wolf 359. 1 smaller red star on a background of starry space.

Wolf 359

A small red dwarf star located in the constellation Leo, it is 7.86 ly from the Sun.

An illustration of Lalande 21185. 1 smaller red star on a background of starry space.

Lalande 21185

Part of the constellation Ursa Major and the brightest red dwarf in the northern hemisphere, it is 8.30 ly from the Sun.

An illustration of Sirius. 1 larger blue star and 1 smaller white star on a background of starry space.

Sirius

The brightest star in the night sky, Sirius is actually a binary system. A bright blue star accompanied by a white dwarf, they are 8.71 ly from the Sun.

An illustration of Gliese 65. 2 smaller red stars on a background of starry space.

Gliese 65

A pair of red dwarf flare stars, variable stars that can undergo unpredictable changes in brightness, they are 8.72 ly from the Sun.

Illustration of a the Milky Way spiral galaxy with a labeled scale of 90,000 light-years across.
The Milky Way Galaxy.

Now let’s take a big step back and look at the Milky Way. Our galaxy is over 90,000 ly in length and Sagittarius A*, the black hole at the center, is about 26,000 ly from us.38

90,000 ly is about eight hundred fifty quadrillion (850,000,000,000,000,000) km. I’ve got nothing to compare that to. We aren’t driving that, probes aren’t flying that, and even the douchebags who own everything don’t have that kind of money. It’s hard not to lose all perspective at this point. Might as well say the galaxy is ten million gazzillion km in diameter because that makes about as much sense to me.

With galaxies needing so much space, there must be like what? 7 or 8 of them out there? Well, no. There are somewhere between 200 billion (200,000,000,000) and 2 trillion (2,000,000,000,000) galaxies in the observable universe,39 and they are all absurdly far from one another. In the mid 1990s, NASA pointed the Hubble Space Telescope to a tiny piece of space no bigger than a person’s thumbnail would appear on their outstretched arm, about one 24-millionth of the whole sky. They left the telescope pointed to that one location for days to collect as much light as possible and see as far into space as possible. The image they got revealed a sea of galaxies gradually fading into oblivion.40

icon of a video Source: NASA’s Goddard Space Flight Center; Lead Producer: Paul Morris

The Milky Way is over 90,000 ly in diameter, holds hundreds of billions of stars in its giant spiral arms, and is still just a speck of dust in an ever-growing universe of mostly empty space. But have fun at work tomorrow.

Parsec (pc)

You had to know a new unit of measurement was coming, right? You can’t see the Hubble Deep Field (HDF) image and not immediately think: Damn, my usual way to measuring distances would be meaningless in a place like this. How would I measure it? Great question. Let’s look at the parsec (pc).

A two-panel comic featuring cartoon versions of Han Solo and Chewbacca. Top panel: Han Solo confidently says, "It’s the ship that made the Kessel run in less than 12 parsecs." Chewbacca stands next to him, smiling. Bottom panel: Han says, "Nerds will now spend the next few decades thinking the parsec is a measurement of time." Chewbacca maintains the same expression.

A parsec is not that much bigger than a light-year, 1 parsec = 3.26 light-years, but it’s handy in defining big distances because, like meters, you can add prefixes to it and multiply its value exponentially.

  • 1 parsec (pc) = 3.26 light-years (ly)
  • 1 kiloparsec (kpc) = 3,261.56 light-years (ly)
  • 1 megaparsec (Mpc) = 3,261,563.78 light-years (ly)

So although the Milky Way is over 90,000 ly in diameter, that is only about 27.5 kpc. Every time the values start to get unmanageable, our old friend science kicks the door in with a new unit of measurement. Huzzah for science! 🎉🔭🎉 Why do we use megaparsecs instead of light-centuries and light-millennia? No idea.

I mentioned earlier how the Milky Way would one day collide with the Andromeda galaxy. That’s because we are both part of a local group of galaxies known as the Local Group (again, brilliant!). So far we’ve counted about 80 galaxies and it covers a distance of roughly 3 Mpc (10,000,000 ly).41 With gravity’s help, every star in this group will eventually be in one giant galaxy. I’ve heard the name Milkdromeda used to refer to it. Yeesh! At least we’ll all be dead, amiright everyone? *waits for high five*

The Local Group is part of a cluster of galaxy groups known as the Virgo Supercluster, which has an estimated diameter of 33 Mpc (110,000,000 ly) and contains at least 100 galaxy groups and clusters.42 It’s like Russian nesting dolls, you keep pulling back and you get bigger and bigger structures made of stars.

3D map of the Local Group and nearby galaxies, centered on the Milky Way. Nearby galaxies are labeled and connected by lines to show their positions in space. Concentric rings indicate distances up to 8 million light-years.
Local Group and nearest galaxies.
icon of an image Illustration by Antonio Ciccolella. Via Wikimedia Commons. This image is licensed under the Creative Commons Attribution-Share Alike 4.0 International license.

Local Group

Home of the Milky Way. Who names their local group of galaxies the “Local Group”? Kinda dickish, no? Can’t be bothered to find some fun astrological / mythological name or anything? Did you name your cat, Cat?

Cool name score: 1/5

Galaxies: ~30

Diameter: 3 Mpc

Virgo Supercluster

Home of the Local Group. Also known as the Local Supercluster. No seriously, look it up. What is it with these scientists? No imagination. I hear it referred to as Virgo Supercluster more often so they get a pass. For now.

Cool name score: 3/5

Galaxies: ~47,000

Diameter: 33 Mpc

Laniakea Supercluster

Home of the Virgo Supercluster. Now this is what I’m talking about. “Laniakea or laniākea is a Hawaiian word that means ‘immense heaven’, ‘open skies’, or ‘wide horizons’.” Yes! Exactly! No notes!

Cool name score: 5/5

Galaxies: ~100,000

Diameter: 160 Mpc

Pisces–Cetus Supercluster Complex

Home of the Laniakea Supercluster. Supercluster Complex does sound pretty metal and Pisces–Cetus has some mystique. -1 for not using Cletus when it was right there.

Cool name score: 4/5

Galaxies: ~1,000,000

Diameter: 300 Mpc

A map of the nearby universe showing the distribution of galaxy superclusters and voids within 100 million light-years. The Milky Way is at the center. Various superclusters, such as Virgo, Coma, Centaurus, Pisces-Cetus, and Shapley, are labeled in cyan. Voids like the Sculptor Void, Bootes Void, and Capricornus Void are labeled in red. The image is surrounded by a roughly spherical distribution of white filaments representing galaxy clusters. Coordinate markers and gridlines are overlaid in blue for reference.
Pisces–Cetus Supercluster Complex. The universe within 1 billion light years of Earth, showing local superclusters. Approximately 63 million galaxies are shown.
icon of an image Illustration by Richard Powell. Via Wikimedia Commons. This image is licensed under the Creative Commons Attribution-Share Alike 2.5 Generic license.

The Virgo Supercluster is in an even bigger supercluster named the Laniakea Supercluster. At around 160 Mpc (520 million light-years) in diameter, this giant supercluster is estimated to contain over 100,000 galaxies,43 each of which able to produce billions or even trillions of stars.

Once we go back far enough, we start to see that the universe’s galaxies occupy what looks like giant filaments of matter. Often compared to a spider web or the neurons in a person’s brain, these enormous structures are separated from one another by even bigger voids and supervoids of mostly empty space.

The biggest structure of named galaxies we are part of (that I could find) is the Pisces–Cetus Supercluster Complex. The estimates I found put its diameter at around 300 Mpc, almost 1 billion light-years.44 No references left. Just look at the awesome illustration by Richard Powell. Can you see your house?

Illustration of a yeti (head and shoulders only) in front of a flower pattern.
YETI SIDEBAR
We aren’t part of it, but the biggest structure in the universe we have observed is the Hercules-Corona Borealis Great Wall. An absurdly large filament of the cosmic web, this is where the universe’s earliest galaxies formed and flourished. It is estimated to be 10 billion light-years wide, 7.2 billion light-years long, and 1 billion light-years thick.45

So how big does it all get? Can the universe just keep going on forever? Well, it might. Truth is, we aren’t all that sure. Our best science says there was a start to the universe (Big Bang46) about 13.8 billion years ago and it has been growing bigger ever since. So, with that, we could say there is a border or rim around it all, but again its just too big for us to know for sure.

The observable universe is the part of the Universe that we can actually see, and its nowhere near the whole thing.

“No signal can travel faster than light, hence there is a maximum distance, called the particle horizon, beyond which nothing can be detected, as the signals could not have reached the observer yet.”47

– Wikipedia

We very strongly believe the universe keeps going beyond what is observable but we will never see it. The universe keeps expanding and all the giant clusters of galaxies are moving away from each other so we can see less and less of the far universe everyday. More space is being made right now but less of it is visible to us. Eventually, only the stars in our Local Group will be available to us, everything else will be beyond our reach.

A logarithmic-scale map of the observable universe showing the cosmic web of galaxies as white filaments on a black background. The center of the image is labeled "Virgo Supercluster (Milky Way)" in green. Concentric ellipses represent distances from the Milky Way, with labels marking "1 billion light years" and "1 billion parsecs." A white circle marks the outer boundary labeled “Observable Universe Limit.” The full diameter of the observable universe is shown as "93 billion light years / 28 billion parsecs." Coordinate lines and angular measurements from 0° to 180° are overlaid in cyan and white.
Illustration of the observable universe. The scale is such that the fine grains represent collections of large numbers of superclusters.
icon of an image Illustration by Andrew Z. Colvin. Via Wikimedia Commons. This image is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.

In conclusion

Space is wicked cool! It can make us all seem so insignificant (I mean, look at all that space), but without finding life anywhere else so far, it also makes us the most significant things in this giant universe. The only place where real meaning, thought and love can exist.❤️ Plus tacos, sushi, anime, sex, and weed.

Notes & references

  1. R: Neutron Star. (2025, March 4). In Wikipedia. https://en.wikipedia.org/wiki/Neutron_star
  2. R: Red Dwarf. (2025, March 1). In Wikipedia. https://en.wikipedia.org/wiki/Red_dwarf
  3. R: Universe. (2025, March 2). In Wikipedia. https://en.wikipedia.org/wiki/Universe
  4. R: Sun. (2025, March 6). In Wikipedia. https://en.wikipedia.org/wiki/Sun
  5. R: Moon Fact Sheet. NASA Space Science Data Coordinated Archive. https://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html
  6. N: 360,000 km at 120 km/h = 3,000 hours (or 125 days).
  7. N: Venus is sometimes referred to as Earth’s twin (or sister planet) because they are similar in size, density, and composition.
  8. R: Venus. (2025, March 13). In Wikipedia. https://en.wikipedia.org/wiki/Venus
  9. N: 41,000,000 at 120 km/h = 341,666.67 hours (or 14,236.11 days or 39 years).
  10. R: Orbit of Mars. (2025, February 24). In Wikipedia. https://en.wikipedia.org/wiki/Orbit_of_Mars
  11. R: NASA Mars 2020 Perseverance Cruising at 24,600 MPH on Its 300 Million Mile Journey to Mars. (2020, August 1). scitechdaily.com https://scitechdaily.com/nasa-mars-2020-perseverance-cruising-at-24600-mph-on-its-300-million-mile-journey-to-mars
  12. R: Hohmann transfer orbit. (2025, January 21). In Wikipedia. https://en.wikipedia.org/wiki/Hohmann_transfer_orbit
  13. R: Mars 2020 Perseverance Landing Press Kit. NASA Jet Propulsion Laboratory. https://www.jpl.nasa.gov/news/press_kits/mars_2020/landing/
  14. N: That’s what she said.
  15. R: Astronomical unit. (2025, March 12). In Wikipedia. https://en.wikipedia.org/wiki/Astronomical_unit
  16. N: 299,792,458 meters per second (in a vacuum). The fastest speed possible in our universe.
  17. N: Are you thinking 8x 1 min. sessions? Nope, wrong. 1st session is quick and it gets progressively slower (and more painful) as I proceed.
  18. N: Forever my boo, Pluto.❤️
  19. R: Voyager 2. (2025, March 26). In Wikipedia. https://en.wikipedia.org/wiki/Voyager_2
  20. R: Kuiper Belt. (2025, March 19). In Wikipedia. https://en.wikipedia.org/wiki/Kuiper_belt
  21. N: 67.86 AU × 8.317 min/AU ≈ 564.4 minutes (or 9hrs 24min).
  22. R: Solar irradiance. (2025, March 16). In Wikipedia. https://en.wikipedia.org/wiki/Solar_irradiance
  23. N: 0.296 / 1361 * 100 = 0.0217.
  24. N: Full Moon ≈ 0.25 lux. Converted ≈ 0.001–0.002 W/m2.
  25. R: Moonlight. (2025, March 21). In Wikipedia. https://en.wikipedia.org/wiki/Moonlight
  26. R: Voyager 1. (2025, March 23). In Wikipedia. https://en.wikipedia.org/wiki/Voyager_1
  27. R: Scattered Disc. (2025, March 14). In Wikipedia. https://en.wikipedia.org/wiki/Scattered_disc
  28. N: Comets are sometimes referred to as dirty snowballs, due to Fred Lawrence Whipple’s “icy conglomerate” hypothesis of comet composition (later called the “dirty snowball” hypothesis)
  29. R: Oort Cloud. (2025, March 29). In Wikipedia. https://en.wikipedia.org/wiki/Comet
  30. N: 86400 seconds in a day. 365.25 days in a year. 1,000,000 / 86400 = 11.5 days. 1,000,000,000 / 86400 = 11,574.07 days (or 31.68 years). 30,000,000,000,000 / 86400 = 347,222,222.22 days (or 950,642.63 years).
  31. R: Proxima Centauri. (2025, March 26). In Wikipedia. https://en.wikipedia.org/wiki/Proxima_Centauri
  32. R: Andromeda–Milky Way collision. (2025, March 15). In Wikipedia. https://en.wikipedia.org/wiki/Andromeda%E2%80%93Milky_Way_collision
  33. N: \(\frac{4.01 \times 10^{13} \ \text{km}}{1.39 \times 10^6 \ \text{km}} \approx 2.89 \times 10^7 \approx 29 \ \text{million}\).
  34. R: Parker Solar Probe. (2025, March 18). In Wikipedia. https://en.wikipedia.org/wiki/Parker_Solar_Probe
  35. N: \(\frac{4.01 \times 10^{13} \ \text{km}}{6.9 \times 10^5 \ \text{km/h}} \approx 5.81 \times 10^7 \ \text{hours}\) (or 58,100,000 hours or 6,633 years).
  36. R: NASA’s Parker Solar Probe Makes History With Closest Pass to Sun. science.nasa.gov. https://science.nasa.gov/science-research/heliophysics/nasas-parker-solar-probe-makes-history-with-closest-pass-to-sun/
  37. R: List of nearest stars. (2025, March 29). In Wikipedia. https://en.wikipedia.org/wiki/List_of_nearest_stars
  38. R: Milky Way. (2025, March 28). In Wikipedia. https://en.wikipedia.org/wiki/Milky_Way
  39. R: Galaxy. (2025, March 24). In Wikipedia. https://en.wikipedia.org/wiki/Galaxy
  40. R: Hubble Deep Field. (2025, March 1). In Wikipedia. https://en.wikipedia.org/wiki/Hubble_Deep_Field
  41. R: Local Group. (2025, April 1). In Wikipedia. https://en.wikipedia.org/wiki/Local_Group
  42. R: Virgo Supercluster. (2025, March 7). In Wikipedia. https://en.wikipedia.org/wiki/Virgo_Supercluster
  43. R: Laniakea Supercluster. (2025, March 20). In Wikipedia. https://en.wikipedia.org/wiki/Laniakea_Supercluster
  44. R: Pisces–Cetus Supercluster Complex. (2025, March 18). In Wikipedia. https://en.wikipedia.org/wiki/Pisces%E2%80%93Cetus_Supercluster_Complex
  45. R: Gamma-ray bursts reveal largest structure in the universe is bigger and closer to Earth than we knew: ‘The jury is still out on what it all means.’ (2025, April 20). Space.com. https://en.wikipedia.org/wiki/Big_Bang
  46. R: Big Bang. (2025, March 18). In Wikipedia. https://en.wikipedia.org/wiki/Big_Bang
  47. R: Observable universe. (2025, March 24). In Wikipedia. https://en.wikipedia.org/wiki/Observable_universe