There seems to be a wide discrepancy, which puzzles people out of Trek, just like me, like me.
The exact reference for the photon torpedoes is as follows:
The Expense, season 2.[Armoury]
REED: Photonic torpedoes. Their range is over fifty times greater than our conventional torpedoes, and they have a variable yield. They can knock the comm. array off a shuttlepod without scratching the hull or they can put a three kilometre crater into an asteroid.
TUCKER: How long is it going to take to reconfigure the tubes?
REED: We've got three teams working on it. They promise me it'll be done before we leave Spacedock, but I've got to start integrating them into the power grid.
TUCKER: Let's go.
First, Reed mentions conventional torpedoes. What's this? Did the NX-01 use photon torpedoes, or more of these conventional torpedoes? The shift happened around season 2, that's it?
Secondly - and that's the big part - why does there seem to be such a huge difference of yields?
There's enough evidence in Trek to show that torpedoes are used just as much as phasers, if not less.
We've found evidence, from dialogue posted in the versus debates, that they're largely unfocused weapons, and actually require manual tweaking to release their energy in a cone.
I tried to know if there was a way to make the 3 km wide crater claim fit with sub megaton yields.
The question is how to obtain a reliable figure for that. Either from a calculator, or from real life examples.
Using M. Wong's calculator, with the results under "cratering energy".
There's a problem though, because the mechanism that leaves a crater due to an impact with a massive object has nothing to do with the mechanism of a small torpedoes liberating enough energy, omnidirectionally (even modern Trek torps around TNG aren't focused), to actually dig a crater that is 3 km wide. There's not the massive residual mass of an asteroid to be meshed with the ground.
See, the idea was to use the cratering figures for a 3000 wide asteroid impact, as it "seemed" to suit the case:
"Cratering energy is the energy required to blast out a crater of depth equal to the radius of the asteroid, which should easily result in its catastrophic disruption."
However, with craters due to asteroid impacts, the width is largely superior to the depth.
There's like a good load of sites to ponder this:
http://www.lpl.arizona.edu/SIC/impact_c ... rater.html
http://www.lpl.arizona.edu/SIC/impact_c ... tpage.html 30-50 meters wide asteroid: a mile wide and 570 feet (173.736 m) deep crater. Yield: 20-40 MT.
http://www.lpl.arizona.edu/SIC/impact_c ... ppage.html
http://www.lpl.arizona.edu/SIC/impact_c ... opage.html 30-50 m wide asteroid: 1 km wide, 100 m deep crater. Yield: A hundred times more powerful than the Hiroshima blast.
http://www.lpl.arizona.edu/SIC/impact_c ... tsmap.html
So I tried Wong's calculator. Recent data has shown that his equations disputable when it came to fragmentation energies (omni blast from the center of an asteroid), and that even with melting a vast bulk of an asteroid, this wouldn't even allow the creation of small enough debris, but would let, instead, to the fragmentation of large plates to be hurtled away.
Here, I tried first a 1000 wide asteroid. A 500 m radius. Same for the depth then.
Result: Even the hardest of materials, nickel-iron, only returns a yield of 4.7 megatons.
So according to his program, a ground blast of 4.7 MT would already be enough to dig a 500 meters deep crater into a surface of nickel-iron, while the estimations I link to say that even blasts between 20 and 40 MT weren't even able to leave craters more than 100-174 m deep, in what is nothing more than granite, as far as Africa is concerned, and let's not mention Arizona's rock.
So I decided to input a 200 m wide asteroid. Radius, 100 m, used for the depth, again.
Cratering energies
- Hard Granite: 180.9 tons
- Nickel-Iron: 4.7 kilotons
So we see that the resulting estimations, as far as it goes for cratering figures, are erroneous.
A way to make sense of this is to suggest that his calculator assumes a rather spherical crater, maybe slightly flattened, but not by much.
But let's do a final test. Frankly, I thought that was an OK way to reach sub megaton yields. We see that in the examples mentionned above, that a crater's final depth is generally a tenth of its width.
So for a 3 km wide crater, we'd get a depth of 300 meters.
Though Wong's program, it gives us those values:
Cratering energies
- Hard Granite: 4.9 kilotons
- Nickel-Iron: 127.5 kilotons
As far as hard-granite is concerned, the yield doesn't come far ahead of the cannons stuck on a maximum of 500 GJ x 10 (overload) each. With two fore phase cannons, we're in a total yield in the 2.39 KT per salvo, per second (I'm unsure as to how long the beam weapons can't be kept firing at maximum power).
The Enterprise is said, early in the show, to have 14 beam weapon spots, a few of them being major cannons like the ones mentionned above.
So, the situations are:
- The pages I've linked to are severely wrong when it comes to yield estimations (or relies on a definition of "crater depth" due to an asteroid impact that is different than the one which corresponds to the crater depth described on Wong's page), but we need to reinterpret the meaning of certain elements and assume that the crater left on the surface of the fictional asteroid mentionned by Reed will share the same kind of shape as a post-asteroid-impact crater. Thus, we obtain ranges from low kiloton to medium kiloton level warheads, which establishes a level of consistency that is satisfying.
- Wong's calculator is largely flawed (or relies on a definition of "crater depth" that is different than the one which corresponds to the depth of a crater left by an asteroid impact), and ENT Trek torps are easily in a range around 40~60 MT, if not more. But then we're still left with that illogical gap of warheads being many thousand times more powerful than beam weapons, and yet rarely used despite the NX-01 facing head to head, numerous times, much more powerful enemies.
Episodes like the Aenar really disputes the vast differences of yields.
Any thoughts?
PS: that's my first Trek centric thread ever; go easy with me guys. :P