How Big is Our Universe?

How Big is Our Universe?

We are tiny creatures, living out short lives in an immense and ancient universe.  We’ve evolved to make sense of the scales of time and space that were relevant for survival of our ancestors, so it is remarkable that we have any inkling at all of just how small we are when we zoom out to the cosmic scale.  As Douglas Adams wrote in ‘The Hitchhiker’s Guide to the Galaxy’:  

Space is Big.  You just won’t believe how vastly, hugely, mind-bogglingly big it is.  I mean, you may think it’s a long way down the road to the chemist’s, but that’s just peanuts to space.”  

To try to make sense of the vast distances between the stars and galaxies, lets scale down the universe.  It is remarkable that even when we shrink things down quite a lot, we find that it is difficult to keep the sizes from rapidly becoming astronomical once again.  This exercise also helps make clear why interstellar travel is such a difficult prospect, and may be nearly impossible to accomplish, even for a very advanced civilization.  This is some of the fun you can have on a Saturday afternoon with some imagination, a calculator, and an understanding of how to use scientific notation.   So, lets begin!

All right, for our first scale down cosmos we will shrink our sun down to the very manageable size of a 1 inch marble.  That’s pretty small right?  That is about 2 one hundred billionths of the suns actual size.  So, with a 1 inch marble at the center of our solar system, here is what follows.  The innermost planet in our solar system, Mercury would be in orbit 3.5 feet from the sun, Venus would orbit at 6.5 feet, and Earth would be a tiny 0.23mm speck (barely visible) sitting 9 feet from the sun.   Next comes the planet Mars sitting 13.6 feet from the sun.  This is our inner solar system, and so far still pretty manageable – a solar system you could fit fairly easily in your living room.

  Next comes the outer solar system with the mighty Jupiter, a speck of 2.5mm flying around the sun at 46 feet from our marble sun.  Beautiful ringed Saturn is in orbit at 85 feet, Uranus at 172 feet, and Neptune at 269 feet.  Little Pluto, now sadly demoted to a dwarf planet, is in orbit at 354 feet.  From that distance our little marble sun would appear tiny, yet it’s the gravitational pull on the tiny dust mote of Pluto that keeps it chained to the solar system.   No longer can we hold the outer solar system in our living room.  We might need to move our solar system to the park to hold it all.  

Think for a moment of how empty our solar system really is.  Tiny specks of dust orbiting a tiny star.  Our model 1 inch sun holds almost all the mass in the solar system.  The rest is just a scattering of microscopic dots out hundreds of feet from the center, with mostly emptiness between them.  The solar system is really very very empty, indeed.

The New Horizon space probe, our fastest space craft yet, visited Pluto last year, taking nearly 10 years to make the trip from Earth.   How fast can we possibly get through the solar system.  Light, traveling at the fastest speed possible in the vacuum of space moves, you guessed it, at the speed of light.  At our little solar system scale the light leaving the sun would take 8 minutes just to pass the Earth 9 feet away.  After an hour of travel the photons of light would move only 64 feet through our little solar system.  That would be somewhere between the orbit of Jupiter and Saturn.  Think of a sphere of light traveling in all directions from our 1 inch sun and taking a full hour to move to a sphere with a radius of 64 feet.  That seems rather slow, but there is nothing known in the universe that can do better.

On this scale 1 light year (the distance that light travels in one year) would be 107 miles from our little sun, and the closest star to the sun – Proxima Centauri at 4.24 light years away – would be a staggering 454 miles out.   Our little 1 inch sun floating alone in the darkness of space with next closest marble sized star being over 450 miles out in the distance.  If the sun marble was located in Los Angeles, then Proxima Centauri would be located approximately at 100 miles further north than San Francisco.   Is it any wonder that interstellar travel is such a monstrous challenge?  To travel between the stars on human time scales seems like an unrealistic dream.

The star Trappist-1, which was recently in the news for having been confirmed to have 7 exoplanets in orbit around it (some of which are in the starts habitat zone)  At a mere 40 light years from earth it has been toted has being very close to us indeed.  On the scale of our model solar system  Trappist-1 would be a small marble 4226 miles from our sun.  Again, if our sun was in Las Angeles then Honolulu would be only 60% of the way out to where the little marble of Trappist-1 would have to be placed – that vast Pacific wildness becoming the vast empty ocean between the stars.  

From our model sun, the center of the Milky Way galaxy would be 2,675,000 miles away, or about 11 times further out than our moon.   The size of the galaxy from end to end would be 10,700,000 miles across.  The next large spiral galaxy to us is the Andromeda galaxy and that would be placed 271,000,000 miles away.  Now that is getting into scales that match the sizes found in our actual solar system.  For example, if our marble sun was sitting in the very center of our actual sun, the surface of the real sun would be 4040 light years on our scale model.  The mini Andromeda galaxy would be beyond the orbit of Mars.

Ok, time to change our scale model to make the universe more manageable again.  Lets suppose that instead of our sun being 1 inch in diameter, our entire Milky Way galaxy is just 1 inch in diameter.  On this scale the Andromeda galaxy is another small disk (a little larger than our Milky Way) just 2.1 feet away from us.  The Virgo cluster of galaxies, which contains thousands of galaxies would be 54 feet away, and the edge of the observable universe, 46.6 billion light years away, would be 7.35 miles in every direction from our little 1 inch disk galaxy.  I’ve heard of races where runners run “the solar system” and pass the orbits of planets at the appropriate places on their 10K race, but you could do a “Run the Universe” race too, where you run a 10K and pass, not only deeper into space but farther back into time until you reach the very edge of time and space at the finish line.   By the way, even though the universe is only 13.8 billion years old the edge is 46.6 billion light years away because the universe expanded much faster than the speed of light in the distant past.  Inside the disk of our tiny 1 inch galaxy, the distance from the Sun to Pluto would be just 1.59 Angstroms, which is very nearly the size of a Hydrogen atom.

What if we wish to make our entire observable universe the size of a friendly 6 inch diameter snow globe, so we can put it out on our desk and admire the whole of creation as we do our work?  What would that look like?  If the observable universe was 6 inches in diameter, then the Milky Way galaxy would be a speck in the very center of the globe (yes, we are in the center of the universe from our vantage point) that was a mere 160 nanometers across.  This would be approximately the size of a virus.  In fact, all the hundreds of billions of galaxies in your Observable Universe globe would be the size of viruses.  I’m not sure you would see anything when you looked in your snow globe universe since the galaxies themselves would be microscopic on this scale, but you could surely feel quite satisfied that when you held your snow globe every galaxy in the observable universe was in the palm of your hand! 

Fossil Friday: Thar She Blows; Whale evolution.

Thar She Blows: Evolution of whales!

by Rich Feldenberg

 

Welcome back to Fossil Friday.  The evolution of the cetacean group (marine mammals like whales and dolphins) is one of the coolest and most beautiful demonstrations of a clear link of fossil evidence from primitive forms to modern forms with many transitional fossils present.  

Whales, are of course, mammals and descended from air breathing land vertebrates.  All tetrapods descended from lobe finned fish (see my Tiktaalik post).  From there they diversified into amphibians, reptiles, mammals, and birds.  Some of the groups of reptiles (like the great marine reptiles during the age of the dinosaurs), and mammals (like the whales) returned to the sea many millions of years later.  Based on molecular genetics studies, the closest living land mammals to the whales is the hippopotamus.  
Cute little Pakicetus was one of the earliest known proto-whales.  These hoofed footed mammals were alive about 50 million years ago.  Based on bone structure of the skull around the auditory region, they fit into the cetacean group, but were not thought to be good swimmers.  Good swimmers in the family would come later!
It is thought that changes in the regulation of genes such as Sonic Hedge Hog (Shh) and Tbx4 may have been important in the loss of the hind limbs in the cetaceans.  By affecting when and how genes are expressed, major changes in structure can be made due to relatively small genetic changes. It is also pretty amazing to see the embryology of modern whales also betrays their ancestry. For example, in the whale fetus the nostrils start out in the usual position for a mammal, but as the maxillary bones grow to huge proportions this forces the nasal bones to the top of the skull. This type of evolutionary effect is called allometry and refers to a change in body parts due to changing the growth rate of different parts in relation to one another.
Over time the cetaceans evolved their characteristic echolocation apparatus, as well as, the development the blow hole from nostrils that were originally forward on the face.  Today, cetaceans are beautifully adapted for life in the oceans.
References and a cool video to watch:
1. Whale evolution Wikipedia:
2. Animated video of whale evolution. This is pretty cool, check it out.
3. Sonic hedge hog:  Wikipedia

Atomic Tuesday: The Magic Numbers of Nuclear Physics

Atomic Tuesday:  The Magic Numbers of Nuclear Physics.
by Rich Feldenberg

Similar to the way electrons reside in atomic orbitals around the atom, the protons and neutrons that make the atomic nucleus are also organized into orbitals or shells.  The Nuclear Shell Model addresses the structure and energy levels associated with these nuclear shells.  No two protons or neutrons (nucleons) can be found in the same shell if they contain the same quantum state (again very similar to the quantum rules followed by electrons going into atom orbitals- Pauli exclusion principle). 

Each energy shell can hold up to a certain “magic number” of protons or neutrons, but all nucleons within the shell must be of different quantum states.  If all the quantum states for that shell are already taken, then they will go to the next available shell.  The magic numbers are 2, 8, 20, 28, 50, 82, and 126 – indicating the number of nucleons possible in each of the shells.  If an atom happens to contain a magic number or protons or neutrons it is found to be very stable, and these also correspond to atoms that are the most prevalent in the environment.   An example would be element 10 (2 for the first shell plus 8 for the second shell).  Element 10 is neon which is a stable nucleus.

If an element has both a magic number of protons and a magic number of neutrons it is “doubly magic”, and has a tightly bound nucleus.  An example would be Lead-208, which has 82 protons and 126 neutrons.  Heavy elements like lead (Pb) usually have more neutrons than protons since the electrostatic repulsion of the protons needs to be balanced out by more neutrons which provide the strong nuclear force to keep the nucleons bound together.

References:
1. The Nuclear Shell Model; University of Nebraska

2. The Nuclear Shell Model: University of California

3. The Nuclear Shell Model – Wikipedia