daytime observing: sun, noon, south

Daytime Observing: Sun, Noon, South

Starry Monday

• On Monday, Science 237

• 7pm lecture “The Planets”

• 8pm rooftop observing

• Show up for either to get 2% credit

Sun Measurement - 01

• We measured at 11:30 am on Jan 29, 2014

• Length of the shadow of a meter stick was 1.72m

• Trigonometry: 30.2 degrees (sig figs!)

Sun Measurement - 02

• We measured at 2:00 pm on Jan 29, 2014

• Length of the shadow of a meter stick was 1.69m

• Trigonometry: 30.6 degrees (sig figs!)

Is this good or bad or what?

• Compare to expected value:– Westerville location 40° N latitude– Celestial equator 90° off of that

• “that” being North AND 40° above horizon

– Sun’s celestial (not observer!) coordinates on January 29: -18°, i.e. south of Celestial Equator (see YourSky)

– So: 40° + 90 °+18 ° = 148° above N horizon

= 32° above S horizon

Define Noon

• I.e. agree on the word “noon” meaning (being equivalent to) “time when the sun reaches the highest altitude in the observer’s sky”

• Note that this time is – different when you are further east or west– the same when you are further north or south

• Note that the sun culminates in the North in the southern hemisphere!

Define South

• Either opposite of direction to the North Star

• Or: direction in which the sun culminates

Why are Polaris and the Sun in opposite directions?

• They are not exactly, because “the north direction” and “the south direction” do not exist

• Their positions are related because – the direction of Polaris defines the rotation axis of

the celestial sphere– The sun is somewhere on the sphere– From a “skewed” perspective everything on the

sphere culminates on the meridian

Reminder: Observer Coordinates

• Horizon – the plane you stand on

• Zenith – the point right above you

• Meridian – the line from North to Zenith to south

What you see depends on where you are!

• Your local sky – your view depends on your location on earth

Constellation 1: Orion

• “the Hunter”

• Bright Stars: D) Betelgeuze E) Rigel

• Deep Sky Object:

i) Orion Nebula

Constellation 2: Gemini

• “the Twins”

• zodiacal sign

• Brightest Stars:

I) Castor

J=K) Pollux

Constellation 3: Taurus

• “the Bull” • zodiacal sign

• Brightest Star: F) Aldebaran

• Deep Sky Object:

iii) Plejades

Constellation 4: Ursa Major

• Other name:

Big Dipper• Stars:

B) Dubhe

C) Merak

• Navigation: go 5 times the distance from Merak to Dubhe and you are at Polaris.

Constellation 5: Ursa Minor • Other name:

Little Dipper

• α Ursa Minoris is

Polaris [A], the pole star

Constellation 6: Canis Major

• “Big Dog”

• Stars:

H) Sirius (brightest fixed star)

Constellation 7: Cancer

• “Crab”

• No bright Stars

Constellation 8: Leo

• “the Lion”

• zodiacal sign

• Brightest Star:

G) Regulus

Constellation 9: Cassiopeia

• Greek mythological figure: mother of Andromeda

• the big “W” in the sky

• No bright stars

Constellation 10: Pisces

• “the Fishes”

• Zodiacal sign

• No bright stars

Constellation 11: Pegasus• Greek

mythological figure: the winged horse

• big rectangle in the sky

• No bright stars

Constellation 12: Andromeda• Greek mythological

figure: Daughter of Queen Cassiopeia and King Cepheus rescued from Cetus by Perseus

• Deep Sky Object:

Andromeda Galaxy

Position: Angles vs. Distances

• Locations in the sky are easy to measure: 2 angles

• Distances from observer are hard (one length)

Together they give the location of an object in three-dimensional space

Angles and Angular Size

• Angles measured in degrees– full circle = 360; right angle = 90– 1 = 60' (minutes of arc or arc minutes)

– 1' = 60" (seconds of arc or arc seconds)

• Typical angular sizes: – Moon 0.5 Sun 0.5 Jupiter 20”, Betelgeuse (α Ori) 0.05”

The Trouble with Angles

• Angular size of an object cannot tell us its actual size – depends on how far away it is

• Sun and Moon have very nearly the same angular size (30' = ½) when viewed from Earth

Without Distances …

• We do not know the size of an object

• This makes it hard to figure out the “inner workings” of an object

• We can’t picture the structure of the solar system, galaxy, cosmos

The most important measurement in Astronomy: Distance!

• The distances are astronomical!

• The distance scales are very different– Solar system: light minutes– Stars: light years– Galaxies: 100,000 ly– Universe: billions of ly

• Need different “yardsticks”