Download Celestial Objects

Celestial Observations
Celestial Coordinates
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Celestial Sphere 1 – Many ancient societies believed the sky was an immense, hollow
sphere surrounding the Earth. They imagined the stars, planets, Sun, and Moon
attached to this sphere and rotating around the stationary Earth every 24 hours.
Although it is now known that this ancient model is incorrect, it is still a convenient
way to predict the motions of celestial objects relative to a location on the Earth.
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Celestial Dome 1 – As you look at the sky, it appears like a large dome over your
head. You are seeing half of the celestial sphere; the other half is below the
horizon. The celestial dome defines the local sky (the sky as seen from wherever
an observer happens to be standing).
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Horizon – The boundary between the Earth and the sky.
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Zenith 2 – The point directly overhead, wherever an observer stands 3.
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Celestial Meridian 4 – An imaginary line that starts at the north point of the horizon,
goes to the zenith, and from the zenith, to the south point of the horizon.
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Celestial Poles 5 – The projections of the Earth’s north and south poles onto the
celestial sphere, thus creating the north celestial pole (NCP) and the south celestial
pole (SCP).
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Precession 6 – The Earth behaves somewhat like a spinning top, causing the axis
of rotation to trace out a circle. This slow conical motion of the Earth’s axis of
rotation is called precession, and is due to the gravitational effects of the Sun and
Moon on the Earth’s equatorial bulge. Precession slowly alters the direction of
the polar axis, causing the gradual apparent shift of the NCP and SCP. This
causes the “pole” stars – any bright star that happens to be within a few degrees of
the NCP and SCP – to be represented by different stars at various times.
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North Pole Stars 7 – At the present time, Polaris in Ursa Minor is the North
Star. About 5000 years ago, the star Thuban in Draco was the North Star,
whereas 13,000 years from now, the star Vega in Lyra will be the North Star.
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One “wobble” (360) of the Earth’s axis of rotation equals 25,725 years
(1  72 years).
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Celestial Equator 8 – The projection of the Earth’s equator onto the celestial sphere.
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Ecliptic 9 – The apparent path of the Sun through the sky. This path corresponds to
the zodiac constellations, the set of constellations through which the Moon and
planets also appear to move. Because it’s the Earth and not the Sun that is actually
moving, the ecliptic corresponds to the plane of the Earth’s orbit 10.
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Celestial Positioning
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Distances 11 – All celestial objects appear to be attached to the celestial sphere, but it
is an illusion. In other words, we lack depth of perception when we look into space,
and therefore it looks like all celestial objects lie at the same distance.
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Distances to objects within the solar system can be measured in miles.
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The Moon – The Moon is the closest celestial object to the Earth at a distance
of about 238,000 miles.
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The Sun – The Earth is the third planet from the Sun at a distance of
approximately 93,000,000 miles.
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Neptune – Neptune is the planet furthest from the Sun (and the Earth) at a
distance of approximately 2,800,000,000 miles.
Light Year – Because the distances to stars are so vast, using the mile as a unit of
distance is inappropriate. Instead astronomers use light years. Light travels at a
speed of about 186,000 miles per second in the vacuum of space, and therefore
can cover a distance of nearly 6,000,000,000,000 (6 trillion) miles in one year.
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Proxima Centauri 12 – A member of the Alpha Centauri triple system, Proxima
Centauri is the nearest star to us at a distance of 4.22 light years
(approximately 25 trillion miles).
Horizon System 13 – When locating celestial objects in the sky, a useful frame of
reference is the horizon. The “horizon system” divides the celestial dome into
imaginary lines referred to as altitude and azimuth.
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Altitude 14 – The celestial object’s angular height above the horizon. The altitude
of a celestial object can be measured in degrees or fractions.
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Azimuth 14 – The celestial object’s compass direction along the horizon. The
azimuth of a celestial object can be measured in degrees or common terms.
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On the horizon = 0
At the zenith = 90
1/2 = 45
1/3 = 30
2/3 = 60
North = 0
East = 90
South = 180
West = 270
The horizon system is only viable for a particular latitude and longitude. For
example, the altitude of a particular star would be quite different if viewed from
the North Pole, Equator and South Pole 15.
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The location of the celestial poles (and celestial equator) is dependent upon the
observer’s latitude.
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Northern Hemisphere – The altitude of the north celestial pole (Polaris) equals the
observer’s latitude.
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Southern Hemisphere – The altitude of the south celestial pole equals the
observer’s latitude.
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North Pole (90N) 16 – The NCP is directly above (located at the zenith).
Equator (0) 17 – The NCP is on the north horizon (and the SCP is on the
south horizon).
40N 18 – The NCP is 40 above the north horizon.
30S 19 – The SCP is 30 above the south horizon.
Differences in latitude not only change the altitude of the NCP (Polaris) and the
SCP, but all celestial objects 20, 21.
Celestial Motions
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Diurnal Motion 22 – The daily rising in the east and setting in the west of celestial
objects. Diurnal motion is caused by the Earth’s rotation.
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Seasonal Motion 23 – A slower cycle of the Sun and stars (constellations) from east to
west can be observed. This cycle brings back the same stars to the same place at the
same time each year. Therefore, each season is characterized by a particular group of
constellations. The seasonal motion is a manifestation of the actual orbital motion
(revolution) of the Earth around the Sun.
Celestial Objects
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Stars – A star is a massive, gaseous body held together by gravity and generally
emitting light. Normal stars generate energy by nuclear reactions (fusion) in their
cores.
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Constellations – A constellation is a pattern of stars that is identified by a given
name. They usually represent mythological gods, people, animals, or objects. An
example of a constellation is Orion, the hunter 24.
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The word constellation is derived from the Latin language, meaning “with
stars”. The origin of constellations is a very archaic concept, created during
the times of prehistory. Many cultures developed their own constellations.
However, we are most acquainted with the constellations based upon the
Greek myths.
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Constellations were confined to the outlines of their identifying forms. Stars
lying outside these forms were called “unformed” or “scattered” (Egyptians)
or “outside the image” (Arabians). However, in 1930, the International
Astronomical Union adopted standardized boundaries for all the recognized
constellations; the formerly adjacent stars are included in these areas.
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“Twinkling” Stars 25 – Stars shine with a steady light. However, starlight coming
through the Earth’s turbulent atmosphere causes the star to appear to twinkle.
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Magnitude – A scale of measuring brightness in which each magnitude jump
represents a 2.512 factor increase or decrease in brightness. The larger the
number, the fainter the star. The magnitude scale can include fractions, zero, and
negative numbers. For example, a –1.5 magnitude star is 100 times brighter than
a +4.5 magnitude star.
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Apparent Magnitude (m) – The brightness of a star as seen from the Earth is
dependent upon: (1) the star’s luminosity, which is the total energy it actually
emits per second in all directions and (2) the star’s distance from the Earth
(the inverse square law of light propagation, B = 1/d2).
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Planetary Objects – Apparent magnitudes are also assigned to planetary
objects (planets and the Moon). Like stars, the apparent magnitude of a
planetary object is dependent upon distance. However, it is also due to the
planetary object’s albedo, which is the amount of light reflected by the
planetary object compared to the amount of light received. Generally, a
large albedo indicates an atmosphere, water, and/or ice (snow).
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The brightest celestial object is the Sun with an apparent magnitude of
–26.78. The Moon is second: m = –12.5. Venus is third: m = –4.6.
The brightest star is Sirius: m = –1.4, whereas Polaris = +2.0.
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The faintest celestial object that the naked eye can discern is about +6.5.
Absolute Magnitude (M) – The magnitude that a star would appear to have if
viewed from a distance of 32.6 light years (10 parsecs). For example, the Sun
has an absolute magnitude of +4.8, whereas Sirius: M = +1.0. Absolute
magnitude allows astronomers to measure the energy output of stars.
Circumpolar Zone (Window) 26 – The region of the sky that the stars and
constellations always appear above the horizon. The size of this zone is
dependent upon the observer’s latitude.
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Long Island (40N) 27 – The circumpolar zone is within 40 of Polaris.
There are five constellations that are circumpolar for Long Island or any
location at a latitude of 40N: Ursa Minor, Draco, Cepheus, Cassiopeia, and
Camelopardalis.
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North Pole – The circumpolar zone is the entire sky, and therefore all
constellations observed are always above the horizon.
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Equator – There is no circumpolar zone, and therefore all constellations rise
and set.
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The Sun – The Sun is a star. However, it is a special star because it’s the one the
Earth orbits. The Earth’s revolution around the Sun, coupled with the planet’s axis of
rotation being tilted by 23.5 to the ecliptic plane 28, causes the seasons. The seasons
relate to changes in the rising and setting positions of the Sun and the Sun’s angular
height and the amount of time it spends above the horizon 29.
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Summer – The Sun rises in the northeast and sets in the northwest, and it’s high in
the sky and days are long.
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Winter – The Sun rises in the southeast and sets in the southwest, and it’s low in
the sky and days are short.
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Spring and Fall – The Sun rises in the east and sets in the west, and it’s halfway
between the highest and lowest points and days and nights are equal in length.
Planets – Today, the term planet is defined as an object in orbit around a star.
However, this ancient Greek word originally meant “wandering star”, because they
appeared to shift amongst the stars of the zodiac constellations.
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Five planets are easy to find with the naked eye: Mercury, Venus, Mars, Jupiter,
and Saturn. Uranus is just visible without optical aid, but you need a dark sky to
succeed, while Neptune requires a telescope to be observed.
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The planets are named after the rulers among the gods in Roman mythology.
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Planets shine, for the most part, with a steady light. The size of a planet in the sky
“averages out” the turbulent effects of the Earth’s atmosphere, presenting a
relatively stable image to the eye.
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Planets increase and decrease in brightness. This change in brightness is due to
the varying distances of the planets from the Earth.
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Non-Uniform Motion – Planets increase and decrease in speed.
(The cause of non-uniform motion will be discussed later.)
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Annual Motion 30 – Planets appear to gradually shift west to east with respect to
the stars. This shift is called annual motion and is due to a planet’s orbital
motion.
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The Sun and Moon also shift west to east with respect to the stars. The Sun’s
shift is due to the Earth’s orbital motion around the Sun, whereas the Moon’s
shift is due to its orbit around the Earth.
Retrograde Motion 31 – At various times, the planets reverse their course and
appear to shift east to west with respect to the stars. This shift is called retrograde
motion. (The cause of retrograde motion will be discussed later.)
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It is during retrograde motion that a planet appears its brightest 32.
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The Moon – The Moon is the Earth’s natural satellite. However, the term “moon”
can be used to refer to a natural satellite of any planet.
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Lunar Phases 33 – The changes in phases of the Moon occur because light from
the Sun illuminates one half of the Moon, and as the Moon orbits the Earth we see
varying amounts of the Moon’s illuminated half.
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The first calendars were based on the cycle of lunar phases, hence the word
“month”.
Eclipse – The blockage of light from one celestial object caused by the passage of
another between it and the observer.
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Solar Eclipse 34 – The passage of the Moon between the Earth and the Sun so
that our view of the Sun is partially or totally blocked.
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Lunar Eclipse 36 – The passage of the Earth between the Sun and the Moon so
that the Earth’s shadow falls on the Moon.
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Moon’s Shadow 35 – Taken in 1999 by the Mir space station, the image
shows the Moon’s shadow darkening part of the Earth during a solar
eclipse.
Red Moon – The Moon appears reddish in color because the Earth’s
atmosphere bends some of the red light from the Sun around the Earth and
toward the Moon.
Rarity of Eclipses 37 – Eclipses are rare because the Moon’s orbit around the
Earth is tilted with respect to the Earth’s orbit around the Sun. Without the
tilt, we would have solar and lunar eclipses every month. However, with the
tilt, the result is that at new moon, the Moon’s shadow generally falls either
above or below the Earth, and at full moon the Earth’s shadow falls above or
below the Moon. Therefore, eclipses only occur when the Moon’s orbital
plane “points” at the Sun.
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