How the Sky Moves Evening Classes Week One Presented by Oisín Creaner.

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How the Sky Moves Evening Classes Week One Presented by Oisín Creaner

Transcript of How the Sky Moves Evening Classes Week One Presented by Oisín Creaner.

Page 1: How the Sky Moves Evening Classes Week One Presented by Oisín Creaner.

How the Sky Moves

Evening Classes

Week One

Presented by Oisín Creaner

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Course Outline

Week 1: The Sky

Week 2: The Planets

Week 3: The Stars

Week 4: History of Astronomy

Week 5: Telescopes

Week 6: Deep Sky Objects

– Week 7: Cosmology

Week 8: Alien Worlds

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Basic Equipment

•Your eyes!

•Binoculars

•Books

•Planisphere

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What can I see?

•Stars & Constellations

•The Planets (W2)

•Galaxies & Nebulae (W6)

•The Moon and Sun (CAREFUL!)

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The night sky is like an up-turned bowl above theastronomer’s head.

a: Zenith

b: Meridian

c: Horizon

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We can pretend thenight sky is a sphere,because all its starsare so far away fromus, they don’t appearto move at all.

The Celestial Sphere

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The Celestial Sphere appears to spinbecause we see it from the surfaceof the spinning Earth.

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Stars appear fixed on the Celestial Sphere.

The Plough

Polaris

Orion

Note the positions of –

•The Plough

•Polaris

•Orion

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Celestial Coordinates

Declination is equivalent to latitiude and is measured in degrees.

Right Ascension is equivalent to longitude and is measured in hours, minutes and seconds.

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Special Observation Locations

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The View from Athlone - 53° North

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Polaris stays in the same place –always directly North, 53° above the horizon.

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Where you are on the Earth’s surface determineswhat constellations you can see, and how often.

Declination ofstars seen from Athlone

Circumpolar –90° N to 37° N

Seen sometimes –37°N - 37°S

Never seen – 37°S - 90°S

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The ecliptic is where the Sun is seen againstthe Celestial Sphere.

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The zodiac is a 16º wide band of sky wherethe planets are seen.

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Ecliptic

γCel. Equator

The Sun crosses the celestial equator at the firstpoint of Aires, in the constellation Pisces.

This is the zero-point of the RA axis (0h 0m)

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The Sun’s movement above & belowthe Celestial Equator

The track of the Sun across the Celestial Sphereis known as the Ecliptic.

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Precession ofthe Equinoxes

The spinningEarth wobbles on its axis once every 26,000 years.

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Using A Planisphere

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PolarisTime

Date

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Match the timewith the date

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The Sky Window

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Autumn Sky- October 10 p.m.

Since there are 12 months in the year, and 24 hours in the day, every month, an object will rise 2 hours earlier

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Autumn Sky- Andromeda

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Autumn Sky- Andromeda

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Autumn Sky- Cygnus ‘The Swan’

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Autumn Sky- Sagittarius ‘The Teapot’

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Canis Major

Canis Minor

Gemini

Auriga

Taurus

Orion as a signpost

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Thank You

www.astronomy.ie/handoutswww.stellarium.org

Useful websites