Interaktiivsed matemaatika- ja teadusõppetunnid (ﾉ◕ヮ◕)ﾉ*:･ﾟ✧
Astronoomias ei mõõdeta peaaegu midagi otse. Kaugused, massid ja temperatuurid tuletatakse heledusest, värvusest ja ajastusest, ning just see järelduste ahel ongi tegelik aine.
Lühikesed jadad üksikute tööriistade asemel. Iga samm annab järgmisele midagi kindlat, seega tasub need läbida järjekorras.
L2: kool
ASTROTähe kohta ei saa tema näiva heleduse põhjal midagi välja arvutada enne kui sa tead, kui kaugel ta asub. Need neli käivad just sellises järjekorras. Ja täpselt sama rada pidi on liikunud astronoomia — iga redelipulk mõõdetud vahetult madalama astme järgi teel maamõõtja kolmnurgast kuni vaadeldava universumi piirini välja.
L3: ülikool
ASTROOrbiidi määravad selle suurus ja kuju. Peaaegu kõik muu tuleneb otseselt neist. Need viis tööriista viivad meid ellipsist kütuseni: kus kosmoselaev asub, kui kiiresti see liigub, kui kaua lend kestab, milline teekond on soodsaim ning kui palju kulub selleks rakettkütust.
The Sun pulls the Moon twice as hard as the Earth does
The Earth pulls the Moon with 1.98 × 10²⁰ newtons. The Sun pulls it with 4.35 × 10²⁰. The Sun wins by more than two to one, the Moon stays with us anyway, and the reason is not the one most people reach for.
The night sky should be as bright as the Sun. Step outside and check.
If the universe were infinite and eternal, every direction you look would eventually hit a star, and the night sky would glare like the surface of one. It is dark instead, and the darkness is evidence about the age of everything.
Nobody has ever weighed the Sun. We timed something going round it instead.
There is one way to measure a mass you cannot touch: watch something orbit it, and time the orbit. The same equation weighs planets, stars and whole galaxies. Dark matter turned up where its answer stopped matching the sky.
A quasar at z = 3 is receding at 1.46 times the speed of light
Cosmological redshift is not a Doppler shift, and the difference stops being academic above z ≈ 1.5, where the recession speed exceeds c without anything moving through space or breaking relativity.
To catch the spacecraft ahead of you, slow down
Firing your engine towards a target in the same orbit sends you further behind it. The only way to catch up is to brake, drop into a lower and faster orbit, and come back up in front.
Most of a rocket is fuel, and better engineering will not change that
The rocket equation is logarithmic in the wrong direction: speed goes up like the logarithm of the mass you carry. Reaching orbit costs more than everything after it.
