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Venus Faser

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Submitted By Miehaugaard
Words 572
Pages 3
Venus’ faser
Formål: At se hvilket verdensbillede, der beskriver Venus bevægelse mest korrekt . Er det det heliocentriske verdensbillede eller det geocentriske verdensbillede?

Teori:
Venus har faser. Ligesom månen ser Venus ikke altid rund ud, når man ser i en kikkert.

Geocentrisk og heliocentrisk verdensbillede:
Det geocentristiske verdensbillede, Ptolomæus verdensbillede, hvor Venus og de andre himmellegemer/planeter bevæger sig i epicykler rundt om jorden. Her er Jorden verdens stillestående centrum, hvorom Solen, stjernerne og planeterne bevæger sig; i modsætning til heliocentrisk verdensbillede, Kopernikus’s verdensbillede, hvori Solen er centrum og planeterne er i cirkelbaner rundt om.

Fremgangsmåde:
Apparatur og materialer
Tennisbold (Venus)
Lampe (Solen)
Øje (Jorden)
Målebånd
Vinkelmåler
Lineal

Apparatur og materialer
Tennisbold (Venus)
Lampe (Solen)
Øje (Jorden)
Målebånd
Vinkelmåler
Lineal

For at lave forsøget skal vi lave en model af solsystemet. Vi skal bruge en tennisbold, som symboliserer Venus, en lampe, som symboliserer Solen og vores eget syn, som skal bruges til at se Venus i forhold til jordens placering. Dernæst skal vi placere solen (lampen) 149,6 cm fra placeringen af vores øje (Jorden). Målestoksforholdet er, at 1 cm svarer til 1 mio. km. Herefter afsættes den første vinkel 40 grader, og Venus (bolden) placeres langs vinklens ben indtil man fra Jorden ser den ønskede fase på Venus (som vist på billedet). Man gør på samme måde med de andre vinkler (48-, 35- og 41 grader). Vi skal huske at bemærke, at det kan være nødvendigt at dreje lampen, således at ”solens” stråler rammer direkte på Venus.

Resultater:
Skema af måleresultater: Dato | Vinkel | Afstand fra Venus til Solen | Afstand fra Venus til Jorden | 07/07-04 | 40 grader | 126 cm | 45 cm | 17/08-04 | 48 grader | 105 cm | 87 cm | 05/11-04 | 35 grader | 123 cm | 148 cm | 15/09-05 | 41 grader | 108 cm | 150 cm |

1 cm = 1 mio. km.

Databehandling – Resultat beregninger:

Diskussion:
De første resultater vi fik af omløbstiden var 791,71 dage, det tog for Venus at tage en bane rundt om solen. Resultatet af omløbstiden skulle have været 219 dage (0.61 år) ud fra den sideriske omløbstid (den tid det tager for at Venus tager en omgang rundt om solen). Grunden til den store variation mellem resultaterne, kan være en målefejl eller en vurderingsfejl under udøvelsen af forsøget. Målingen af de to første vinkler skal ikke være ret meget forkert for at have give et helt forkert resultat (som her - vores udregninger er rigtige). Dog kunne vi se ud fra vores sidste beregninger af vinklerne 48 og 35, at det ville tage 488,31 dage for Venus at tage en runde om solen. Dette passer bedre overens med det rigtige resultat end de første målinger. Her var vores øjemål mere præcise.

Hvis Venus cirkulerede rundt om Jorden, hvilket det geocentriske verdensbillede referer til, så skulle afstanden mellem Venus og solen være varierende. Derimod hvis Venus bevægede sig rundt om Solen, hvilket det heliocentriske verdensbillede siger, så ville afstanden mellem Venus og solen være konstant.

Konklusion:
Vores formål med forsøget var at se hvilket verdensbillede, der beskriver Venus bevægelse mest korrekt . Vi ville finde ud af om det var det heliocentriske verdensbillede eller det geocentriske verdensbillede? Ud fra vores beregninger og måden vores punkter for Venus var placeret, kan vi konkludere, at Venus bevæger sig omkring solen og ikke Jorden. Dvs. at det heliocentriske verdensbillede er det korrekte.

Fejlkilder: * Upræcise målinger med målebånd * Upræcise beregninger * Upræcise vurderinger af, hvor meget tennisbolden/Venus er oplyst

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