Docsity
Docsity

Prepare for your exams
Prepare for your exams

Study with the several resources on Docsity


Earn points to download
Earn points to download

Earn points by helping other students or get them with a premium plan


Guidelines and tips
Guidelines and tips

Lunar Motion and Phases: Understanding the Moon's Orbit and Phases - Prof. Phillip J. Mart, Study notes of Astronomy

An overview of lunar motion and phases, including the moon's orbit around earth, its angular diameter, and the causes of its changing appearance throughout the month. It also discusses the difference between the sidereal and synodic periods and explains how the moon's position in the sky changes over time.

Typology: Study notes

2009/2010

Uploaded on 12/07/2010

lockwooda3
lockwooda3 🇺🇸

2 documents

1 / 42

Toggle sidebar

Related documents


Partial preview of the text

Download Lunar Motion and Phases: Understanding the Moon's Orbit and Phases - Prof. Phillip J. Mart and more Study notes Astronomy in PDF only on Docsity! 1-4: Lunar Motion & Phases Image Courtesy of Mike Kozma Earth & Moon Earth Sun 0.5o Angular diameter of the Sun viewed from Earth is likewise 0.5o. Earth Sun 0.5o Angular diameter of the Sun viewed from Earth is likewise 0.5o. Moon is much closer! 390 km 384,000 km 10 1.5 Moon to Dist Sun to Dist 8    Your index finger, held at arm’s length, subtends about 1o - 2o. Lunar Motions Moon’s orbit – viewed from above Earth’s north pole: counterclockwise  Orbit period = 27.3 days (Sidereal Period) Far side Near side Cha Sy tele Rotation Period = 27.3 days Moon’s rotation period = its orbital How it would be IF Moon did not period. It keeps ane side facing the Earth. rotate. Sametimes we would see We never see far side of Moon (shaded), far side of Moon. Moonsync.mov (Moon Rotation Movie) [Exit ‘show’ mode; right click on caption; select ‘package object/activate contents.’] Orbit Orbit, viewed edge-on: Earth’s orbit plane Moon ’s orb it plan e 5o Moon’s orbit plane is tilted slightly relative to Earth’s orbit plane. Another view . . . Plane 5o (Line of Nodes) View From Earth Viewed from Earth, moon moves ~ 13o/day E S W 9 pm9 pm9 pm 13o 13o Because Earth’s orbit & the Moon’s orbit are tilted by 5o, the Moon is never more than 5o from the ecliptic . . . . . . consequently, rising & setting points wander only a little more than Sun’s rising & setting points. Lunar Phase Cycle A Anen ea Gres ae re ' Horizon Bees cieim elie rsa Horizon: . . : : ‘. care Sera esaraken Yi cae . ; Third (Last) Quarter . ee Sera eV korres ae { a an cs ae Aaa _ eC Po . i. 7 One eae 7 - ; a ; a a aa Sunlight Note: Not to scale Earth Moone.g., First Quarter View from Earth Result: Moon appears one-half illuminated The Moon’s phase (synodic) period is longer than its orbit (sidereal) period: 29.5 d > 27.3 d To distant stars Lunar Phase Visibility At what time of day are the various phases visible in your sky?
Docsity logo



Copyright © 2024 Ladybird Srl - Via Leonardo da Vinci 16, 10126, Torino, Italy - VAT 10816460017 - All rights reserved