Steam installeren
inloggen
|
taal
简体中文 (Chinees, vereenvoudigd)
繁體中文 (Chinees, traditioneel)
日本語 (Japans)
한국어 (Koreaans)
ไทย (Thai)
Български (Bulgaars)
Čeština (Tsjechisch)
Dansk (Deens)
Deutsch (Duits)
English (Engels)
Español-España (Spaans - Spanje)
Español - Latinoamérica (Spaans - Latijns-Amerika)
Ελληνικά (Grieks)
Français (Frans)
Italiano (Italiaans)
Bahasa Indonesia (Indonesisch)
Magyar (Hongaars)
Norsk (Noors)
Polski (Pools)
Português (Portugees - Portugal)
Português - Brasil (Braziliaans-Portugees)
Română (Roemeens)
Русский (Russisch)
Suomi (Fins)
Svenska (Zweeds)
Türkçe (Turks)
Tiếng Việt (Vietnamees)
Українська (Oekraïens)
Een vertaalprobleem melden
Horsens, Vejle, Denmark 
🤔
I went on to test the program in every way I could devise. I strained
it to expose its weaknesses. I ran it for high-mass stars and low-mass
stars, for stars born exceedingly hot and those born relatively cold.
I ran it assuming the superfluid currents beneath the crust to be
absent -- not because I wanted to know the answer, but because I had
developed an intuitive feel for the answer in this particular case.
Finally I got a run in which the computer showed the pulsar's
temperature to be less than absolute zero. I had found an error. I
chased down the error and fixed it. Now I had improved the program to
the point where it would not run at all.
-- George Greenstein, "Frozen Star: Of Pulsars, Black
Holes and the Fate of Stars"
🙂
Never make anything simple and efficient when a way can be found to
make it complex and wonderful.
🤐