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Ch 2 The Sky http://www.blinn.edu/brazos/natscience/kbyboth/phys1411-A3cis.html Objectives Use of the celestial sphere and angular measurement Constellation and Star names Introduce the magnitude scale Relative motion of common naked eye objects 2-1 The Stars Constellations vs Asterisms

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Ch 2

The Sky

http://www.blinn.edu/brazos/natscience/kbyboth/phys1411-A3cis.html


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Objectives

  • Use of the celestial sphere and angular measurement

  • Constellation and Star names

  • Introduce the magnitude scale

  • Relative motion of common naked eye objects


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2-1 The Stars

Constellations vs Asterisms

Two ways to name stars

The brightness of stars, apparent visual magnitudes


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Constellations

The “Obvious” View

On a clear dark night we can see stars to 6th magnitude with the unaided eye. Magnitude scales will be explained later.

The human mind by its nature combines these into patterns. This tendency is useful for organization but can lead to misconceptions about the true positions of the stars.

Our ancestors named these groupings in support of their belief systems and oral traditions. Many of the ones we know today originated in Mesopotamina over 5000 years ago.


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Constellations,2

People connected the stars into patterns we call constellations. Names and myths for constellations are culture dependent, but interestingly enough the stars grouped together are frequently similar. Interpretations are different.


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Orion

Al Jabbar the Giant (ancient Syrians)

White Tiger to the Chinese

Prajapati..a stag in ancient India.

Orion is prominent in winter evening sky.


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Astrology-Astronomy,What’s your sign?

While we scoff at the field of astrology now it is not much of a stretch to see why the ancients thought a cause and effect relation existed between the location of heavenly objects and events in their everyday lives. Modern astronomy owes much to the practice of astrology. Many early astronomers and mathematicians made a living casting horoscopes for wealthy clients.

There are 88 constellations . Regions of the sky are now named by the most prominent constellation in the area.


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Orion and Neighborhood

Constellations Near Orion




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Asterisms

Big Dipper a subset of Ursa Major is an asterism, a smaller less well defined grouping of stars.

The great square of Pegasus is another asterism.



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Star names

The brightest stars were named thousands of years ago.

Most of our constellation names come from Greek versions translated into the Latin, but most star names come from ancient Arabic.

Sirius .. The Scorched One,

Capella .. Little She Goat

Alderbaran… Follower of the Pleiades


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Two ways to name stars

Another more useful method uses the name of the constellation and a Greek letter prefix to indicate the relative brightness.


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Magnitude Scale

From brightest to dimmest.

Hipparchus Gk. 160-127 BC

Originally 6 classes.


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Magitude is not a linear scale. It’s a log scale.

The human eye has been replaced by instruments and a scale has been exactly defined.

Vega ~ 0 mag Antares(alpha Scorpio) 0.92

Spica 0.91

Negative I.e. very bright objects are possible

SIRIUS –1.42

Full Moon –12.5

Sun –26.5



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Orion’s belt and Rigel, Selected magnitudes

Mintaka, 2.25

Pg 15

SAO 132071, 3.35

Rigel, 0.18

Saiph , 2.06


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2-2 The Sky and its Motion

The Celestial Sphere The sky at any moment

Celestial Sphere Reference Points

The Sky and Compass points,

The motion of the sky

Precession, north moves around…slowly

Diurnal Motion


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Celestial Sphere reference Points

Zenith-directly over head

Nadir- 1800 away from zenith

North Celestial Pole-directly above the Earth’s north rotational axis

South Celestial Pole-above south pole


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Sky and Compass points

The great circle passing directly overhead and through the celestial poles is your meridian.


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Prime Meridian

The zero reference meridian passes through the observatory at Greenwich, England.


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Arc distances are measured in degrees

900 right angle

e.g.Horizon to Zenith, due north to due east

1800 straight angle: Zenith to nadir, due east to due west


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Approximate angular separations

Width of little finger… ~10

Fist…~100

Caution!!Be careful where youuse #4 .


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Sky from North Pole

Stand on the north pole and the celestial north pole is at your zenith.


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Sky from 600 N Latitude

Walk 300 south and the pole moves 300 north. You are now at 600 N Latitude.


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Sky from 300 N

Move to 300 N Latitude and the North Celestial Pole is 300 up from your northern horizon and 600 north of your zenith.


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The Celestial Sphere, motion

Stars move across the sky from east to west over the course of a night. This is of course due to the rotation of the Earth on its axis towards the east.

 Which stars are directly overhead depends on our location on the Earth.

The relative positions of the stars remain the same. People thought the stars must be attached to a Celestial Sphere surrounding the Earth.





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Circumpolar Stars

The stars above your northern horizon that never set depend on your latitude.

Polaris, North Celestial Pole, is the same number of degrees above the northern horizon as your latitude.


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Astronomy as a survival tool.

The patterns of stars have been stable over time scales large compared to the lifetimes of men and even their cultures. Stars were thought to live forever.

This stability led to the use of stars as navigational guides, and the repeating nature of the times of which stars are visible led to their value as calendars.

Knowing when to plant crops or to break winter camp to meet migrating game is a real survival tool


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Motion of the Celestial Sphere

Long term changes.. Over centuries. Precession

Daily.. Diurnal motion.


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Precession

A top precesses in a conical motion due to the effect of the earth’s gravity.

The Earth precesses due to the combined effect of the Sun and Moon on the bulge at the Earth’s equator.


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North Pole Moves

The precession has a 26.000 year cycle.

4800 years ago the pole was close to Thuban. The pole will be closest to Polaris in ~2100 .


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LONG-TERM CHANGES

A spinning object affected by an outside force will wobble on its axis. This is called precession. This causes the axis of rotation to trace out a circular path. The Earth’s cycle of precession lasts about 26,000 years.

Figure 1.14


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Due to the precession a sidereal year is about 20 minutes longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.


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Daily..Diurnal Motion longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.


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Diurnal Motion longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.


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Diurnal motion longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.


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More diurnal motion longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.

Time laps photograph


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Diurnal Motion,1 longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.

We now know this motion is due to the rotation of the Earth on its axis.

We still use the concept of the Celestial Sphere to learn our way around the sky.

We use angular separations and positions on the sky to discuss the locations of stars.


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Diurnal Motion,2 longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.

Earth’s Orbital Motion

The 24 hour Solar Day , from noon to noon, is the basic social time unit. By definition 1 solar day is 24 hours.

The daily progress of the Sun and other stars across the sky is called diurnal motion.

Each night the celestial sphere shifts a little across the sky.

… a day measured by the star positions is called a sidereal day.


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Sidereal vs Solar Day longer than a tropical year, 365.256 mean solar days. If we did not use the tropical year the seasonal months would change.

Sidus ,latin for star.

The Earth rotates on its axis and revolves around the Sun.

The solar day is 3.9 minutes longer than the sidereal day.A sidereal day is 23h56m long.


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