Welcome to Starry Monday at Otterbein Astronomy Lecture
Welcome to Starry Monday at Otterbein Astronomy Lecture Series -every first Monday of the month. October 3, 2005 Dr. Uwe Trittmann
Today’s Topics • Observing the Planets • The Night Sky in October
Feedback! • Please write down suggestions/your interests on the note pads provided • If you would like to hear from us, please leave your email / address • To learn more about astronomy and physics at Otterbein, please visit – http: //www. otterbein. edu/dept/PHYS/weitkamp. asp (Obs. ) – http: //www. otterbein. edu/dept/PHYS/ (Physics Dept. )
Observing the Planets Saturn Jupiter Uranus Neptune
The Terrestrial Planets • Small, dense and rocky Mercury Mars Venus Earth
The Solar System: Top View
Side view: Inclination of Orbits • Orbits (here: Mars) are very slightly tilted with respect to the sun-earth plane Planets appear close to the path of the sun in the sky, the ecliptic
Planetary Motions • The sky seems to revolve around us because of Earth’s rotation • Additionally, planets move with respect to the fixed stars, that’s why they are called planets (greek: wanderers) • Due to the planet’s movement in their orbit, and Earth’s orbital motion, this additional motion – the apparent motion of the planet as seen from Earth - looks complicated.
Apparent Planetary Motion • Motion as seen from Earth, which itself is revolving around the Sun.
Explanation 1: Ptolemy (~140 AD) • Planets move on circles sitting on circles around Earth geocentric model • dominates scientific thought during the Middle Ages • Longest lasting (wrong) theory ever: 1000 yrs
Epicycles • Ptolemy’s explanation of retrograde motion • About 40(!) epicycles necessary to explain all observations complicated theory
Explanation 2: Copernicus (1473– 1543) • All planets – including Earth – move around the Sun • Planets still on circles needs 48 epicycles to explain different speeds of planets • Not more accurate than Ptolemy Major Work : De Revolutionibus Orbium Celestium (published posthumously)
Correct Explanation: Kepler, Newton • All planets move around the sun according to Newton’s theory of gravity • Kepler’s laws tell us how the orbits look like, and where a planet is in its orbit
Kepler’s First Law The orbits of the planets are ellipses, with the Sun at one focus
Ellipses a = “semimajor axis”; e = “eccentricity”
Kepler’s Second Law An imaginary line connecting the Sun to any planet sweeps out equal areas of the ellipse in equal times
Kepler’s Third Law The square of a planet’s orbital period is proportional to the cube of its orbital semi-major axis: P 2 a 3 a P Planet Orbital Semi-Major Axis Orbital Period Mercury 0. 387 0. 241 Venus 0. 723 0. 615 Earth 1. 000 Mars 1. 524 1. 881 Jupiter 5. 203 11. 86 Saturn 9. 539 29. 46 Uranus 19. 19 84. 01 Neptune 30. 06 164. 8 Pluto 39. 53 248. 6 (A. U. ) (Earth years) Eccentricity 0. 206 0. 007 0. 017 0. 093 0. 048 0. 056 0. 046 0. 010 0. 248 P 2/a 3 1. 002 1. 001 1. 000 0. 999 1. 000 1. 001
The heliocentric explanation of retrograde planetary motion
Inner and Outer Planets • Inner Planets: closer to sun than Earth – Mercury & Venus – Always close to sun in the sky • Outer Planets: further from sun than Earth – Mars, Jupiter, Saturn, Uranus, Neptune, Pluto – Best viewing when opposite of sun in the sky
Inner Planets superior conjunction Inner planet eastern elongation western elongation inferior conjunction Earth
Outer Planets quadrature conjunction Earth quadrature Outer planet opposition
Close Outer Planet Size of planet varies a lot as Earth moves Earth Outer planet
Far-Out Planet Earth Size of planet varies little as Earth moves Outer planet
Mercury • • Color: yellow-golden Brightness: up to – 1 m Size: 10” When to observe: several times a year for short periods • Difficulty: pretty tough, innermost planet, always very close to the sun
Venus • • Color: white Brightness: up to – 4. 5 m Size: up to 40” When to observe: all year, except for period around superior conjunction; either west of the sun (morning star), or east of the sun (evening star) • Difficulty: very easy
Phases of Venus
Phases of Venus Heliocentric Geocentric
Mars • • • Color: orange Brightness: up to – 2. 2 m Size: up to 25” When to observe: about every 2 years Difficulty: very easy around opposition
Mars Opposition 2005 • • Date of opposition: November 7, 2005 Constellation: Aries Date of closest distance: October 30, 2005 Closest distance to Earth: 69. 42 million km (43 million miles, or 0. 46406 AU) • In 2003 (historically close): 55. 8 million km
Mars • Fairly bright, generally not too hard to see • Smaller than Earth • Density similar to that of the moon • Surface temperature 150– 250 K • Day ~ 24. 6 hours • Year ~ 2 Earth years
Apparent Mars Diameter
The Terrestrial Planets Comparable tilt of rotation axis
Martian Seasons
Polar Ice Caps • Watch them grow and shrink in the telescope
Mars Atlas
Mars observations • Look for surface features • Try to determine which side of Mars we see • Polar caps • Seasonal changes • phases
Dust Storms
Jupiter • • Color: yellowish-white Brightness: up to – 2. 5 m Size: 40” When to observe: most of the year, except for some months around conjunction • Difficulty: easy, moons visible in binoculars
Jupiter & Moons
Saturn • • Color: yellowish Brightness: up to – 1. 5 m Size: 20” When to observe: most of the year, except for some months around conjunction • Difficulty: easy, rings and moons visible in small telescopes
Saturn & Moons
Uranus • • Color: greenish Brightness: around 5. 7 m Size: 4” When to observe: most of the year, except for some months around conjunction • Difficulty: challenging, with binoculars
Neptune • • Color: greenish Brightness: around 7. 8 m Size: 2. 5” When to observe: most of the year, except for some months around conjunction • Difficulty: challenging, good binoculars
Pluto • • Color: white Brightness: 14 m Size: star-like, no disk When to observe: most of the year, except for some months around conjunction • Difficulty: very tough, outermost planet, always very far away, very faint; big telescope and several nights to identify
The Night Sky in October • The sun is past autumn equinox -> longer nights! • Autumn constellations are coming up: Cassiopeia, Pegasus, Perseus, Andromeda, Pisces lots of open star clusters! • Mars is getting close to opposition • Saturn is visible later at night
Moon Phases • Today (New Moon, 0%) • 10 / 10 (First Quarter Moon) • 10 / 17 (Full Moon) • 10 / 24 (Last Quarter Moon) • 11/ 1 (New Moon)
Today at Noon Sun at meridian, i. e. exactly south
10 PM Typical observing hour, early October no Moon Mars Uranus at meridian Neptune
South. West High in the sky: The summer triangle
Due North Big Dipper points to the north pole
High up – the Autumn Constellations • W of Cassiopeia • Big Square of Pegasus • Andromeda Galaxy
Andromeda Galaxy • “PR” Foto • Actual look
East High in the sky: Perseus and Auriga with Plejades and the Double Cluster
South • Planets – Uranus – Neptune • Zodiac: – Capricorn – Aquarius
Mark your Calendars! • Next Starry Monday: November 7, 2005, 7 pm (this is a Monday • Observing at Prairie Oaks Metro Park: – Wednesday, October 12 – Friday, November 18 • Web pages: – http: //www. otterbein. edu/dept/PHYS/weitkamp. asp (Obs. ) – http: //www. otterbein. edu/dept/PHYS/ (Physics Dept. ) )
Mark your Calendars II • • Physics Coffee is every Wednesday, 3: 30 pm Open to the public, everyone welcome! Location: across the hall, Science 256 Free coffee, cookies, etc.
- Slides: 56