16.07.2013 Views

Newtonian mechanics

Newtonian mechanics

Newtonian mechanics

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Problem 1.2<br />

8 OPGAVELØSNINGER 36<br />

Metode: Centripetalkraft leveres af snorekraften<br />

Løsning:<br />

S2 = M1ω 2 r2, S1 = M2ω 2 r1 + S2 = 3M1ω 2 r1<br />

Snor knækker ved M1 fordi S1 > S2. ωmax tilfredsstiller S1 = Smax, dvs.<br />

3M1ω 2 <br />

Smax 327N<br />

maxr1 = Smax ⇔ ωmax = =<br />

= 33.02s−1<br />

3M1r1 3 · 0.1kg1m<br />

2. Selv ved uendelig høj ω kan systemet ikke hænge helt vandret pga. gravitation.<br />

1. Givet: MPhobos = 9.4 · 106m, TPhobos = 27540s, jævn cirkelbevægelse<br />

Ukendt: MMars<br />

Metode: Centripetalkraft leveres af gravitationen<br />

Løsning:<br />

MPhobosω 2 rPhobos = G MPhobosMMars<br />

r 2 Phobos<br />

og idet ω 2 = 4π2<br />

T 2 f˚as<br />

MMars = 4π2r3 Phobos<br />

T 2 =<br />

PhobosG ⇔ MMars = ω2 r 3 Phobos<br />

G<br />

4π 2 (9.4 · 10 6 ) 3<br />

(27540s) 2 · 6.668 · 10 −11 Nm 2 kg−2 = 6.48 · 1023 kg<br />

2. Givet: rMars = 1.52rJord, jævn cirkelbevægelse<br />

Ukendt: ˚Ar p˚a Mars (dvs. TMars)<br />

Metode: Kepler<br />

Løsning:<br />

r3 T 2 = kst ⇔ r3 Jord<br />

T 2 =<br />

Jord<br />

r3 Mars<br />

T 2 ⇔<br />

Mars<br />

<br />

rMars<br />

3 TMars =<br />

TJord = (1.52)<br />

rJord<br />

3/2 1˚ar = 1.87˚ar

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!