DocumentCode
3261918
Title
Acceleration due to gravity changes during solar eclipse phases
Author
Zainuddin, Mohd Zambri ; Ambak, Noorul Aini ; Yahya, Mohd Sahar ; Saadon, Mohd Hafiz Mohd
Author_Institution
Phys. Depts., Univ. of Malaya, Kuala Lumpur, Malaysia
fYear
2011
fDate
12-13 July 2011
Firstpage
170
Lastpage
173
Abstract
Every celestial bodies including our Earth having their own gravity field which causing the attractive force towards the object near them. By assuming that the Earth is symmetrical sphere, the strength of the gravity field at any point on the surface of Earth should be proportional to the mass of the planet and inversely proportional to the square root of two of the distance from the center of the planet. The strength of gravitational force can be equalized with the acceleration of any mass in the influence of gravity and the value on the Earth surface, denoted as g, is approximated with standard average value g = 9.8 m/s2. Experiment conducted during two different solar eclipses, Total Solar Eclipse 2009 and Annular Solar Eclipse 2010. For 2009 experiment, the increment from pre-eclipse to the totality is about 18.92%. For the first and second set of experiment in 2010, showing the percentage increase of gravity acceleration from pre-eclipse to the annularity is about 7.51% and 8.59% respectively. This difference in gravity acceleration may cause chicken egg able to stand during the maximum phase of eclipses.
Keywords
eclipses; gravity; AD 2009; AD 2010; Earth surface; annular solar eclipse; attractive force; celestial bodies; chicken egg; gravity acceleration; gravity changes; gravity field; solar eclipse phases; symmetrical sphere; total solar eclipse; Acceleration; Earth; Gravity; Moon; Oscillators; Sun; Newton´s Gravitational Law; Solar eclipse; local gravity; oscillation; simple pendulum;
fLanguage
English
Publisher
ieee
Conference_Titel
Space Science and Communication (IconSpace), 2011 IEEE International Conference on
Conference_Location
Penang
Print_ISBN
978-1-4577-0563-2
Electronic_ISBN
978-1-4577-0562-5
Type
conf
DOI
10.1109/IConSpace.2011.6015876
Filename
6015876
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