NerdGuy Fridays #12: NerdGuy on the Rocks

A Question of Rocks

I recently had the need to look into rock slides for the opening of Miranda Chase #4, Ghostrider. As usual, two simple lines led to a whole field of learning.

“He remained conscious for the next two hundred feet of descent as a [xxx thousand tons of rock swept him toward the valley floor.”…”At the base of the scree slope, the mountain built a [xxx-foot high burial mound.”

Left brackets “[“ are how I note something in my manuscript that I need to look up later but don’t want to stop the flow of writing to do right at that moment. There are other facts that I do have to stop and look up because the answer will affect which direction I take the story. The volume of rock is one of the former kind. But now it was time to unearth the answers.

Weighing Rock

First, how much does rock weigh?

As part of my senior geophysics thesis in college, I had to weigh core sample that we’d drilled out in my field area. Different types of rock have different weights. Think of talc, which is a rock before it’s ground up into a powder, versus a piece of basalt or granite you tossed out of your garden. If you’ve done construction, think of the weight of a sheet of gypsum (another rock) versus a sheet of slate. I can pick up a 4’x8’x1/2” piece of “sheet rock” fairly easily. In my younger days I’d carry them in pairs. I can move a 2’x4’x1/2” piece of slate, if I’m careful and flip it end for end as I go. In my younger days, I may have been stupid enough to lift it, stupid being the operative word.

So, why was I weighing rock? Well, more dense rock also creates a strong gravitational pull. More matter equals more gravity—so denser rock formations under the ground pull down harder. I had the use of a tool called a gravimeter that could measure those minute differences. First I performed a very accurate topological survey. Then a gravimetric survey over the same area. After doing a horrendous amount of math on an incredibly advanced TI-58 programmable calculator that was the envy of my classmates (1977, $125…really dating myself here), I was able to measure the actual variations in the gravimetric field (a whole other topic that I may geek out on someday). I then could computer model (using a program I had to write in BASIC) what was occurring beneath the surface.

TI 58 Calculator
TI 58 Calculator that powered my Geophysics thesis

The Weight of Rock

This is actually much simpler now, plus I required less accuracy for fiction than for geophysics… I used Google.

The very first site I hit included this wonderful information for landscapers.

https://www.hunker.com/12422226/standard-weights-for-crushed-rock-per-meter

  • Solid rock = 2.5 – 3 tons/cubic meter (NerdBonus: a “ton” is 2,000 pounds, a “tonne” is 1,000 kilograms or 2,200 pounds. So we have a mixed English/metric unit here, but I’m going with it rather than converting.)
  • Uniformly crushed rock = 1.6 tons/cubic meter
  • Mixed crushed rock (due to possibly better packing of space) = 1.6 – 2.2 tons/cubic meter
  • Sand and chips (which I don’t care about here, but was interesting) = .92 tons/cubic meter
  • I was very intrigued that all of the following come in the same at 1.07 tons/cubic meter: pea gravel, 1” crushed concrete, recycled asphalt, and 2” sewer filler rock . Pit run gravel (2” or 4”) both weigh in at 1.25 tons (that funny closest-spatial-packing effect evening things out).
  • Landscaping Rock, now we’re talking:
  • 2”-12” rock = 1.25 tons/cubic meter
  • 12-24” rock = 1.18 tons/cubic meter

All right! I’ve walked across scree slopes in the 2”-12” range (not something to do without careful planning and knowledge—neither of which I boasted at the time). I’ve definitely avoided them in the 12-24” category. So, I now have my working weight of 1.25 tons/cubic meter.

How Much Rock

For that I turned to a different website:

https://www.ngi.no/eng/Services/Technical-expertise/Rock-slides

The Norwegian Geotechnical Institute knows a great deal about rock slides. With 174 dead in the last century (most within just 3 events), they have good reason to. A big rock slide in a Norwegian fjord can create town-killing tsunamis. The 2015 movie The Wave is actually a fascinating (and good) movie about this. It’s billed as “Norway’s First Disaster Movie” and earned a nice 6.7 rating on IMDB and 83% on Rotten Tomatoes.

NGI notes that there are actually three distinct categories:

  • Rock fall < 100 cubic meters. This will block a road or train track very nicely.
  • Rock slide = 100-10,000 cubic meters. These only occur on slopes of 50m or more, otherwise there just isn’t enough height to get that much mass moving.
  • Rock flow > 10,000 cubic meters. This caused the devasting tsunamis in 1905, 1934, and 1936.

The scree slopes of the Rockies are truly massive, easily hundreds of meters high in some places and only semi-stable.

How Much Rock

1.25 tons / cubic meter

<10,000 cubic meters (I wanted an event, not a catastrophe.)

These seemed like good working numbers.

So, the first number I wanted was easy: 12,000 tons of rock.

The second was going to take some more thought. How big a mound was created by 10,000 cubic meters?

First I needed to know the natural angle of a scree slope: 32 degrees is typical in the Scottish Cairngorms: http://www.landforms.eu/cairngorms/scree.htm. Close enough for me. My final cone had to have a radius 3 times wider than it was high.

My search for “Calculating the Volume of a Cone” brought up a neat tool right away.

I fooled around with some numbers until I got this result:

Volume of a Cone
Volume of a Cone

Thirty meters wide and ten meters high didn’t sound very impressive as a burial mound. But then I thought about it. 1) That’s a radius of 30 meters, so a diameter of 60 meters. 2) It’s in metric.

English is always better for measurements like this. A burial mound that was 200’ across and 30’ high—way better.

But was there a better descriptor? I started tinkering.

  • A circular base 200’ in diameter = 31,400 square feet.
  • A football field = 47,970 square feet without the endzones. (“Covering two-thirds of a football field…” sounds a little lame.
  • A FIFA soccer field is even bigger, so that wouldn’t help.
  • From my on-going US Coast Guard short story series, I know that an Endurance-class cutter is 215’ long. But that’s long and narrow, so it doesn’t give the right impression.
  • A US Interstate Highway uses a 12’ lane. 200’/12’ = 16 lanes. Hmmm…

Another NerdBonus: according to Quora, the widest highway section in the US Interstate system runs for 22 miles from Katy, TX to Houston, TX. It averages 22 lanes wide and in some places is 26! Excluding toll booths, it’s the widest in the world. (With tollbooths, it’s 50 lanes on the G4 in China.)

But most of us don’t have much experience with picturing a 16-lane highway. I needed something familiar to most people.

  • A baseball field = 400’ x 400’ = 160,000 sq feet. Nope.
  • A baseball infield = 90’ x 90’ = 8,100 sq feet. Closer. Though if you start looking at specifications for the infield and the dirt running track you find out that: 1) maybe 27,000 is a workable number, but 2) there aren’t actually specific rules according to the blogs on mlb.com. So picturing something that’s variable…nah!

“He remained conscious for the next two hundred feet of descent as a eleven-and-a-half thousand tons of rock swept him toward the valley floor.”…”At the base of the scree slope, the mountain built a burial mound—bigger than a baseball diamond but smaller than the dirt running track and three stories high.” Not really helpful. Even without the running track qualifier it seemed clunky.

  • A full-sized school bus is 45’ long. Hmmm…

“He remained conscious for the next two hundred feet of descent as a eleven-and-a-half thousand tons of rock swept him toward the valley floor.”…”At the base of the scree slope, the mountain built a burial mound—wider than four school buses parked end to end and three stories high.”

Yeah, there it is.

UberNerd Note: Yes, I considered the fact that the mound wouldn’t be accumulating on a perfectly flat valley floor, but rather at the foot of the existing 32-degree(ish) scree slope. But I couldn’t think of how doing all that extra math would make these 2 lines in the book any more impactful—rather quite the opposite, so I left truncated cones and other calcs for a different time.

Until next time: Nerd on!

NerdGuy Fridays #11: 3 Twilights

3 Twilights – which do you care about?

It’s 6:30 a.m. You roll over and glance out the window. (Okay, you morning people who’ve been up and writing for an hour can do that. I have one night owl friend who I often trade e-mails with at this hour…as he heads to bed.)

Anyway, you look out the window and it’s getting light, right?

How light?

What do you care? It’s twilight. And the same for evening time.

Not so fast. There are actually three different twilights:

  • Civil – the sun disappears from view. But it lasts for a while. So, they cut off another slice.
  • Nautical – this is when the horizon becomes pretty much useless to mariners (hence nautical).
  • Astronomical – yet when I ran the college planetarium and arranged night viewing with sessions with telescopes, Nautical Twilight was still a total pain, blocking the best viewing with the sun’s brightness.
What exactly defines each one?

Well, if you want to get fussy (I never, ever do that as a NerdGuy):

  • Civil – the sun drops below the horizon and is up to 6 degrees below
  • Nautical – the sun is 6 to 12 degrees below the horizon
  • Astronomical – 12 to 18 degrees below the horizon

Below 18 degrees? Um, we call it “night” just to make sure we’re on the same page.

twilight graphic
A handy, dandy graphic from Wikipedia (c) PMurph5

But some very neat things are going on at this time.

  • During Civil Twilight, the brightest stars and planets appear. We used to play a game in college that we couldn’t go to dinner until someone had spotted the first star during this time after sunset. It helped to know ahead of time the positions of Venus, Jupiter, Saturn, occasionally Mars and Mercury (though they’re typically nautical twilight finds), and the big for or five stars. Sirus the “Dog Star” in Canis Major (the Big Dog constellation) was always a prime candidate because it was prominent in the fall & winter sky. (Did I mention that the combined physics / astronomy department was mostly made up of nerds?)
  • Nautical Twilight is when you can start playing constellation games and pick out Mars.
  • Astronomical Twilight was an awesome time as kids for a game of flashlight tag. You’d catch a hint of someone on the move, but they were now very hard to find and tag with your flashlight (also because the batteries always seemed to be fading by then).
  • Night, of course, is when the Milky Way shines in all its glory and any nerd with a telescope or binoculars and the super awesome Sky Guide app (iOS only, I think) on their phone can start chasing interesting objects…like the space station, various satellites, nebula, globular clusters, and so on.
How the Sun Moves
  • The sun is 0.5 degrees in diameter.
  • Every day it cruises through 360 degrees of a circle through the sky (roughly–because the Earth moves around it, the earth actually has to rotate just a little over 360 to get back to the same place. Would you believe about 1 degree? Because the Earth is progressing 365 days around the sun, so it has to make up 1 and a little degrees per day).
  • So, with 24 hours in a day, the sun moves 15 degrees per hour (360/24).
Measuring the Sky With Your Fist

FUN ASTRONOMY TIP: You can estimate a lot of distances with the back of your hand. Hold your hand up directly in front of you, with the back of it facing you. (This works on most people.)

  • Hold up your pinkie – that’s about 1 degree wide
  • Hold up three fingers – that’s about 5 degrees
  • Your fist – about 10 degrees
  • Forefinger-to-pinkie horns (middle 2 folded under) – if you just relax and let them splay out a bit, that’s 15 degrees. This is how far the sun, moon, or stars will roughly move in an hour. Is something forty-five degrees above the horizon? That’s three finger-horns.
  • Splayed-thumb-and-pinkie – 25 degrees. This fails on people who can’t extend their pinkies properly (but all seem convinced that they can).

What does all this have to do with how long twilight lasts? Well…

How Long are the Twilights?

This is actually a tricky question.

If the sun passes directly overhead at noon (only possible within 23 degrees of the equator–changing seasonally within that area). It will take just a little over a fist-width of an hour to go from sunset to astronomical night. That’s why in the tropics night seems to “fall so abruptly.”

Now imagine you’re at the North Pole on the summer solstice (and imagine that you aren’t falling through the melting ice pack). Move your fifteen-degree (one hour of sun travel) fist along the horizon. Again and again and… Yup. You never get twilight at all.

Where I used to live in Washington State, summertime sunset was a very leisurely affair. The sun travels at a shallow angle. The transition from sunset to astronomical dark was almost 3 hours at midsummer. True darkness was under two hours long.

So, how long is each twilight?

Well, it’s moving about 3 finger-widths per type of twilight (~5 degrees). But it’s doing it on the slant (unless it’s directly overhead at high noon). That slant must slope down far enough to get about 3 finger-widths perpendicular to the horizon (6 degrees below on the vertical, not the slant).

Easy answer? Look up Miranda’s home (or yours) on a website like sunrise-sunset.org/:

Miranda’s Home of Spieden Island, WA

Why Am I Nerding Out on This?

Because in Miranda Chase #4 Ghostrider, coming out on June 28th (just the week after the solstice), the villain needs to work under the cover of true darkness (which isn’t very long at Miranda’s home in mid-summer), but it’s different in other places she must go.

Her first stop, a plane crash in the mountains of Aspen, Colorado. Her next…