Timestream Post: A note from 01.07.2011

7 01 2016

Bulls-eye! 1989 movie "Back to the Future Part II" depicts (invents?) a 60" widescreen, flat-screen TV and correctly hangs it above the mantle nearly 20 years before they were actually invented...

In the spirit of this experiment, I send this message half-a-decade into the future.  (Truthfully, I hope to positively litter the digital timestream with notes, showing that cyberspace may not only connect us through space, but also through time.)

First, my greeting:  Hello, 2016!  This is a year made nearly famous by films such as Back to the Future, Part II – where in 1989 the distant future year 2015 was depicted as a fantastic realm of flying cars, keyless entry, ubiquitous cybernetic implants, widescreen-flatscreen TVs, governmental weather control, 3D movies (without glasses), hoverboards, video calls (Skype?), video eyeglasses, and electronic roofies.

Reading the list five years out, 50% isn’t bad.  Do the remaining few years close the gap?  If not flying cars, do electric cars break the entry barrier at least?  I wonder…

So, what preoccupies me today?  Unsurprisingly, it’s space travel.  The future of space travel, to be precise.  In a move that some may consider pure insanity in the midst of an economic Great Depression, I decided last summer to start a spaceflight consulting firm, which I hope to incorporate and launch in the next few weeks.  To that end, I’ve been building a coalition of industry professionals during the last six months who I hope to become private space pioneers with me, and I entered an abstract for one of the company’s services – spacecraft ergonomics – into the Next Generation Suborbital Researcher’s Conference next month.  The meeting is only the second meeting of its kind, and one I hope will lead to frenetic networking, and ultimately, clients!

I’ve been working with a design studio, Studio Rayolux under brilliant designer Thad Boss, to develop a brand for the company, which I believe I’m calling “Astrowright Spaceflight Consulting.”  We’ll see if it sticks.

So, my question to the future is simply this:  Did it work?  Did the company get off the ground?  Did I get off the ground?  Can industries be forged during a time of economic strife and emerge triumphant?  Inquiring minds want to know!

Until then, take care, faithful readers.  Go for your dreams and never look back!



January 7, 2011.

January 7, 2011. 5:01pm.

Nuclear and Atomic Radiation Concepts Pictographically Demystified

10 10 2013

Greetings, all.  Today I’m attempting a different, largely pictographic approach to demystifying the concept of “radiation” for the layperson.

Despite the hype, radiation is a natural part of our planet’s, solar system’s, and galaxy’s environment, and one that our biology is equipped to mitigate at ordinary intensities.  It’s all actually surprisingly straightforward.

So, without further ado, here goes – a post in two parts…

PART I – Radiation and Radioactivity Explained in 60 Seconds:

The Atom

This is a generic diagram of the atom, which in various combinations of the same bits and parts is the basic unique building block of all matter in the universe:


This somewhat simplified view of an atom is what makes up the classic “atomic” symbol that most of us were exposed to at the very least in high school.

Radioactive Atoms

However, what is almost never explained in school is that each atomic element comes in different versions – slimmer ones and fatter ones.  When an atom’s core gets too large, either naturally or artificially, it starts to radiate bits of itself away in order to “slim down.”  This is called being radio-active.

So, there’s nothing to “radiation” that we all haven’t been introduced to in school.  Radiation is the name given to familiar bits of atoms (electrons, protons, neutrons) or beams of light when they’re being flung away by an element trying desperately to squeeze into last year’s jeans… metaphorically-speaking, of course.

Here is a diagram illustrating this process.  (Relax! – this is the most complicated-looking diagram in this post):


So, when a radioactive element has radiated enough of itself away and is no longer too large, it is no longer radioactive.  (We say it has “decayed.”)

That’s it!

That’s as complicated as the essential principles of radiation and radioactivity get.  It’s just basic chemistry that isn’t covered in high school, (though in my opinion it should be!).

PART II – Take-Home Radiation Infographics

So, in an effort to help arm you against the rampant misinformation out there, here is a collection of simple diagrams explaining what everyone out there seems to get wrong.  (Feel free to promote and/or distribute with attribution!)

First, what’s the deal with “atomic” energy/radiation versus “nuclear” energy/radiation?  Do they mean the same thing?  Do they not?  Here’s the skinny:


That’s all.  “Nuclear” means you’ve zeroed in on an atom’s core, whereas “atomic” means you’re talking about something dealing with whole atoms.  No big mystery there.

Next, here is a simple diagram explaining the three terms used to describe radiation that are commonly misused in the media, presented clearly (click to enlarge):


(Armed with this, you should be able to see why saying something like, “The radiation is releasing contamination!” doesn’t make a lick of sense.)

Now, here is a diagram explaining the natural sources of radiation we’re exposed to everyday on planet Earth:


And here are the basic principles of radiation safety, all on one, clean diagram (click to enlarge):


The End! 

Despite the time and effort spent socially (politically?) promoting an obscured view of this science (or so it seems), there is nothing more mysterious about radiation than what you see here.

Please feel free to contact me with any questions, and remember:  We have nothing to fear but fear itself!

Semper Exploro!

Ultimately, Time Travel is essential for Space Travel

17 04 2011

Long-time readers may note that this blog bounces (veers?) between space-related content and time/temporal physics-related content.  Today, aside from admitting that (not surprisingly) the two topics are primary passions of mine, I’ll tell you why they’re related, and intimately so.

It’s all Einstein’s fault.

After an interstellar trip, a faulty suspended animation chamber reduces an astronaut to an ancient corpse. (From Planet of the Apes; Credit: 20th Century Fox)

Put very simply, according to Relativity: When dealing with events in the universe, it is impossible to separate the distance of space from the passage of time.

This is why astrophysicists and cosmologists speak of actions in the universe occurring and affecting “space-time.”  (Hence the “space-time continuum” that makes such a frequent appearance in sci-fi technobabble.)

What does this mean for us?  Well, in day-to-day experience, not much more than the odd reality that the moon we see is 1 second old.  Similarly, the sun we see is lagging 8 minutes behind us in time.

Why?  Well, it takes the light that bounces off of the surface of the Moon 1 second to cross the 230,000-mile distance between the Earth and Moon to strike the retina of your eye, and it takes 8 minutes for the light that leaves the sun to cross the 93-million mile orbital void to get to Earth and reach your eye.  As a result, we see the Moon and Sun as they appeared when the light left them, not when the light reaches us.

The same can be said of distant stars.  The farther away a star is, the older it is. (Even if it’s 200,000 light years away – then you’re seeing it the way it looked 200,000 years ago.)

So, quizzically, yes – this means that universe we see is actually a horrible garble of apparent objects from intermixed times.  Fortunately for us,  compared to the incredible speed of light, we’re close enough (distance) to everything we need to experience, (e.g., our limbs, food, loved ones, walls, etc.,) so that this time lag is unnoticeable.

But when we start peering out into the rest of the cosmos, this distortion really matters.  Many of the stars we’re studying may have already exploded… but if they exploded a few years ago, we won’t know it until light from the explosion reaches us, which could take millions of years if the star is far away.

Now, let’s take our time-distance thought exercises a step farther and ask what happens if we score the holy grail of the Search for Extraterrestrial Intelligence.  What if, for the sake of argument, we receive and translate a friendly message from an incredibly advanced race of aliens?  And what if, by fortuitous happenstance, they (hoping to aid other, younger life-forms) offer unlimited knowledge to any beings that can meet them on their world, face-to-face?  Well, the offer doesn’t do us more than a hill of beans of good if it takes us 200 years for a multi-generational craft to get there, only to find that the benevolent race has gone extinct due to a problem with their parent star.  We want to reach them as soon as we translate the message.

We want to separate the distance of space from the passage of time.

So, if we can conceptually and technologically conquer time travel, we will have in essence conquered space travel.  If one can manipulate the passage of time, then the time taken to cross the distance of space with any type of propulsion system becomes an almost trivial tally – little more significant than the miles-per-gallon of a modern automobile.

Conventional propulsion systems will get us around in space for the foreseeable future, and more exotic systems will likely take us to the nearest stars.  However, I believe it will be the mastery of time that will transform our race from provincial planet-hoppers to truly savvy, galaxy-trotting, cosmic-colonial game-changers.

Something to think about.

Astrowright Academy and the Classroom of Tomorrow

23 08 2010

Well, just a quick note this morning.  Today is my first day of class as a graduate student in the University of North Dakota’s School of Aerospace Sciences Department of Space Studies program.

So, you could say that my advanced academic push toward becoming an astrowright has begun.  -And in true 21st Century form, as I commute to work, I’ll actually be “attending” a lecture.

University of North Dakota SpSt 541 class lecture #2. Credit: Me.

Here goes nothing.

%d bloggers like this: