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Basic Observations in Astronomy
Classes without Quizzes-Alumni Weekend at Otterbein-
June 8-10, 2007
Dr. Uwe Trittmann
Welcome to
Basic Astronomy
• Possible topics:– Basic observations – Star Maps– Telescopes– The Night Sky in June– Eclipses
Basic Observations in Astronomy• Positions of objects (sun, moon, planets, stars …) • Motion of objects
– with respect to you, the observer
- with respect to other objects in the sky
• Changes (day/night, seasons, etc.)• Appearance of objects (phases of the moon, etc.)• Special events (eclipses, transitions, etc.)
All “in the sky”, i.e. on the Celestial Sphere
What’s up in the night sky? The Celestial Sphere• An imaginary sphere
surrounding the earth, on which we picture the stars attached
• Axis through earth’s north and south pole goes through celestial north and south pole
• Earth’s equator Celestial
equator
Celestial CoordinatesEarth: latitude, longitude
Sky: • declination (dec) [from equator,+/-
90°] • right ascension (RA) [from vernal
equinox, 0-24h; 6h=90°]Examples:• Westerville, OH 40.1°N,
83°W• Betelgeuse (α Orionis) dec = 7°
24’ RA = 5h 52m
What’s up for you?
Observer Coordinates
• Horizon – the plane you stand on
• Zenith – the point right above you
• Meridian – the line from North to Zenith to south
…depends where you are!
• Your local sky – your view depends on your location on earth
Look North in
Westerville
Look North on
Hawai’i
Daily Rising and Setting
• Due to the rotation of the Earth around its axis
• Period of rotation: 1 siderial day= 23h56m4.1s
• 1 solar day (Noon to Noon) =24h
• Stars rotate around the North Star – Polaris
Solar vs Siderial Day
• Earth rotates in 23h56m
• also rotates around sun
needs 4 min. to “catch up”
• Consequence: stars rise 4 minutes earlier each night
• after 1/2 year completely
different sky at night!
Another Complication: Axis Tilt!• The Earth’s rotation axis is tilted 23½ degrees
with respect to the plane of its orbit around the sun (the ecliptic)
• It is fixed in space sometimes we look “down” onto the ecliptic, sometimes “up” to it
Path around sun
Rotation axis
Position of Ecliptic on the Celestial Sphere• Earth axis is tilted w.r.t. ecliptic by 23 ½ degrees
• Equivalent: ecliptic is tilted by 23 ½ degrees w.r.t. equator! Sun appears to be sometime above (e.g. summer
solstice), sometimes below, and sometimes on the celestial equator
The Seasons• Change of seasons
is a result of the tilt of the Earth’s rotation axis with respect to the plane of the ecliptic
• Sun, moon, planets run along the ecliptic
The Zodiac throughout the Year
Example: In Winter sun in Sagittarius, Gemini at night sky; in summer sun in Gemini, Sagittarius at night sky
Constellations of Stars
• About 5000 stars visible with naked eye• About 3500 of them from the northern hemisphere• Stars that appear to be close are grouped together
into constellations since antiquity • Officially 88 constellations
(with strict boundaries for classification of objects) • Names range from mythological (Perseus,
Cassiopeia) to technical (Air Pump, Compass)
Constellations of Stars (cont’d)
Orion as seen at night Orion as imagined by men
Constellations (cont’d)
Orion “from the side”
Stars in a constellation are not connected in any real way; they aren’t even close together!
Understanding and using Star
Maps
• The night sky appears to us as the inside of a sphere which rotates
• Problem: find a map of this curved surface onto a plane sheet of paper
• Let’s explore our turning star map!
Fixed and unfixed Stuff
• The stars are “fixed” to the rotating sky globe They move from East to West and also
from near to the horizon to higher up in the sky
• The Solar System bodies (Sun, Moon, Planets, Asteroids, Comets) move with respect to the fixed stars
• SSB’s have complicated paths: their own motion is added to the overall motion of the celestial sphere
Motion of Sun, Moon and other Planets• All major bodies in the Solar System move around ecliptic
• Slow drift (from W to E) against the background of stars
Reason: All planets move in same plane!
Motion of the Moon• Moon shines not by its own light but by reflected
light of Sun
Origin of the phases of the moon• Moon revolves around the Earth
• period of revolution = 1 month
Phases of the Moon
Phases of the Moon (cont’d)
• Moon rotates around earth in one month
• Moon rotates around itself in the same time
always shows us the same side!
“dark side of the moon” (not dark at all!)
Motion of the Planets
• Along the ecliptic as Sun and Moon
• But: exhibit weird, “retrograde” motion at times
“Strange” motion of the Planets
Planets usually move from W to E relative to the stars, but sometimes strangely turn around in a loop, the so called retrograde motion.
The heliocentric Explanation of retrograde planetary motion
See also: SkyGazer
SkyGazer
• A computer program that simulates the vision of the sky during day and night
Things to observe:• Set your position on Earth: observe how view of
sky changes as you move E,W, N,S• Note the distribution of sunlight on Earth!• Rotation is around Polaris which is not in zenith
SkyGazer
Things to observe (cont’d):• Sun, moon, planets, stars rise (E) and set
(W)
• In the southern hemisphere the sun is highest in the north
• Planets sometimes move backward
• Moon phases
• Planets have phases, too!
Telescopes
• Light collectors
• Two types:– Reflectors
(Mirrors)– Refractors
(Lenses)
Refraction
• Lenses use refraction to focus light to a single spot
Reflection• Light that hits a mirror is
reflected at the same angle it was incident from
• Proper design of a mirror (the shape of a parabola) can focus all rays incident on the mirror to a single place
Newtonian Telescope
• Long tubes (approx. focal length)
• Open at front
• Eyepiece on side
Schmidt-Cassegrain Telescope (CAT)
• Very compact & easy to use
• Closed (Corrector plate)
• Resonably priced
Refractor
• Two lenses -> inverted image
• Long tube (approx. focal length of objective)
• Usually pretty expensive
Binoculars
• Erect image -> good for terrestrial viewing• Prisms needed to produce erect image• Typical specs: 8x60, means magnifies 8x
and objective lens is 60 mm in diameter
A good starting point
• A pair of binoculars and a star map will keep you busy for a long time – anywhere!– constellations – Planets– Moon– Orion nebula– Andromeda Galaxy– star clusters– …
The Night Sky in June
• The sun is at its highest -> shortest nights!
• Summer constellations are coming up: Hercules, Scorpius, Ophiuchus (Snake Bearer), Snake
lots of globular star clusters!
• Center of the Milky Way in Sagittarius
• Jupiter, Saturn & Venus are easily seen
Moon Phases
• 6 / 8 (Last Quarter Moon)
• 6 / 14 (New Moon)
• 6 / 22 (First Quarter Moon)
• 6/ 30 (Full Moon)
Today at
Noon
• Sun at meridian, i.e. exactly south
10 PM
Typical observing hour, early June
• no Moon
• Jupiter• Pluto
(experts only)
Saturn
Venus
South-West
Virgo and
Comawith the
Virgo-Coma galaxy cluster
Virgo-Coma
Cluster
• Lots of galaxies within a few degrees
M87, M88 and M91
Zenith
• Big Dipper points to the north pole
South– Canes Venatici
– Corona Borealis
– Bootes
– Serpens
Globular Star Clusters:• M 3• M 5• M 13
M 5
Galaxies: • M 51• M 101• M 64 (Bl. Eye)
South-East
– Hercules– Ophiuchus– Serpens
Globular Star Clusters:• M 13• M 92• M 12• M 10 …
M 5Summer is Globular Cluster time!
M13: Globular Cluster
South-East
– Ophiuchus– Serpens– Scorpius
Globular Star Clusters:• M 4• M 19• M 62• M 80 …
M 5Summer is Globular Cluster time!
Appendix: Eclipses
Eclipses
• One celestial object hidden by other or in the shadow of another
• Solar eclipse: sun hidden by the moon• Lunar eclipse: moon in earth’s shadow (sun
hidden from moon by earth)• Also: eclipses of Jupiter’s moons, etc.• Most spectacular because moon and sun
appear to be the same size from earth
Solar Eclipses
• Umbra – region of total shadow• Penumbra – region of partial shadow• Totality lasts only a few minutes!• Why isn’t there a solar eclipse every month?
Solar Eclipse
Solar Corona
Question
Why isn’t there an eclipse every month ?
Answer: because the Moon’s orbit is inclined w.r.t. the ecliptic
Lunar Eclipses Moon moves into
earth’s shadow…
…and out of it
(takes hours!)
Partial Eclipse
Not an Eclipse !
Towards Totality
Almost total…
Totality
Totality