Recent submissions

Comment · 5 years ago
Comment · 5 years ago
Yes, one of the central points of his books ("Maps of Meaning", "12 Rules for Life", and "Beyond Order") is that meaning in life is found by taking on personal responsibility. A good starting point is probably his "12 Rules for Life".
Comment · 6 years ago
You will have to register to Scitation and the free access is only temporary.

> Scientists and students in affected regions can now register on Scitation.org to activate temporary free full-text access to content through April 30, 2020.

Comment · 7 years ago
Comment · 7 years ago
Comment · 7 years ago
Comment · 8 years ago
Comment · 12 years ago
Comment · 12 years ago
Thank you very much for this book! As a beginning game developer this was just what I was looking for. After learning how to do rendering, physics, AI and so on I was missing how to put it all together in a proper way. This is a great resource! :)
Comment · 12 years ago
> there's a rotate button when you click through to the detail page.

When rotating some of the images (for example Img 999) it seems to cut the edges of the image off and clicking to zoom doesn't help.

Comment · 13 years ago
Thanks for the post. They are simple but extremely helpful and not always apparent tips. Courtesy and personal conversation gets you a long way.
Comment · 14 years ago
Thank you all for the answers. Yes I suspect that I was a bit quick to jump on the appeal of the faster microcontroller on the Due while I wont really need it at all, especially in the beginning.
Comment · 14 years ago
I am new to Arduino but very interested in starting. So far I have read that the Uno R3 is the best for beginners but now that the new Due is out will this be preferable for a beginner?

From what I've read, the Due is faster and able to handle more things. But is it easier to use compared to the Uno?

Comment · 14 years ago
The gravitational acceleration is equal to G * M/r^2 where G is the gravitational constant (G = 6.67 * 10^(-11) N * m^2/kg^2) M is the mass of Earth (M = 5.97 * 10^24 kg) and r is the radius of the Earth (average radius = 6.37 * 10^6 m).

At the place where he jumped out the gravitational acceleration would roughly be:

g = G * M/((6.37 * 10^6 m) + (39000 m))^2 ~= 9.69 m/s^2

This is not far from the normally used 9.8 m/s^2 and this would of course get larger as he gets closer to the ground.

Comment · 14 years ago
Could you elaborate a bit on your point 1/3? How come the little interest in this subject? Even though it contains no relativistic effects it would seem to have some importance in filling out the complete 'cube' of theories?

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