The Universe on a Large Scale Farther Away • At a distance of 15 million light years we find other small galaxy • The nearest galaxy to the Milky Way is 75,000 light years away (controversial) Q • Toward the constellation Sagittarius Q • Magellanic Clouds Q groups At 50 million light years there is the Virgo Cluster Many thousands of galaxies • Our Local Group and the Virgo Cluster are part of supercluster that Two small galaxies that appear to be clouds to the naked eye has a diameter of 60 million light years • Nearest large galaxy is Andromeda Galaxy, M31 Q Q Q • Farther away are quasars A spiral galaxy similar to the Milky Way 2 million light years away Part of a cluster of 40 galaxies called the Local Group ISP 205 - Astronomy Gary D. Westfall Q X cosmic microwave radiation left over from the Big Bang Lecture 1 1 ISP 205 - Astronomy Gary D. Westfall Q 1 atom/cm3 in our galaxy 1 atom/m3 between galaxies helium (by weight) • The remaining 90 elements are relatively rare Q centers of stars • These elements were ejected when stars used up their hydrogen fuel and exploded • There are 92 naturally occurring elements (atoms) • Evidence has been found for man-made elements up to 118 Q Lecture 1 Carbon, oxygen, calcium, etc. • Hydrogen and helium come from the Big Bang • The remaining elements were “cooked” in the Most of the mass of an atom is in the atomic nucleus The electrons around the nucleus are at a distance 10,000 times the size of the nucleus ISP 205 - Astronomy Gary D. Westfall 2 • The universe is roughly 75% hydrogen and 25% • Air has about 1019 atoms/cm3 • Even atoms are mostly empty Q Lecture 1 Composition of the Universe • Most of the universe is empty Q Black holes? • Beyond the quasars is the The Universe of the Very Small Q Energetic centers of galaxies 3 Supernova ISP 205 - Astronomy Gary D. Westfall Lecture 1 4 The Celestial Sphere Celestial Poles • When we look up it seems that the Earth is the • The points where the axis of center of the universe Q the Earth intersects the celestial sphere are called the north and south celestial poles • The celestial equator lies halfway between the two poles • The circumpolar zone is always above the horizon, day and night Geocentric • The point above your head is called the zenith • Where the sky-dome intersects the ground is the horizon • The sky seems to rotate around us Q Celestial sphere • We know that the Earth’s rotation on its axis every 24 hours causes this illusion but the concept of the celestial sphere is still useful ISP 205 - Astronomy Gary D. Westfall Lecture 1 5 Rising and Setting of the Sun ISP 205 - Astronomy Gary D. Westfall Lecture 1 6 Tilt of Earth’s Axis • The sun does more than just rise and set • It changes position with respect to the background stars Q Approximately 1 degree per day to the east • The sun moves through the celestial sphere along the ecliptic • The ecliptic is not aligned with the equator of the Earth because the Earth’s axis is tilted 23 degrees with respect to the plane of its orbit around the sun • The Earth rotates on an axis tilted 23 degrees from the vertical ISP 205 - Astronomy Gary D. Westfall Lecture 1 7 ISP 205 - Astronomy Gary D. Westfall Lecture 1 8 Planets and Stars Constellations • Not only does the Sun move but the stars, the • The stars form a fixed background • Distinctive patterns of stars have been recognized moon, and the planets move as well • The moon and the planets move with respect to the stars on the celestial sphere • The moon and the planets move on paths close to the ecliptic as well as the sun • The Sun, the moon, and the planets are all found in a 18 degree wide belt in the sky called the zodiac ISP 205 - Astronomy Gary D. Westfall Lecture 1 throughout the ages • These patterns were usually embellished and given names and drawings • These constellations are not necessarily nearby stars but merely appear to be related • Today the term constellation refers to 88 sectors in the sky 9 Constellations in the Sky ISP 205 - Astronomy Gary D. Westfall Lecture 1 10 Galactic Equator • The galactic equator is defined by the Milky Way galaxy • The ecliptic and zodiac are not aligned with the Galactic equator nor with the celestial equator • In fact, the Galactic equator is very different from the ecliptic and the celestial equator ISP 205 - Astronomy Gary D. Westfall Lecture 1 11 ISP 205 - Astronomy Gary D. Westfall Lecture 1 12 Locating Objects on a Skymap Locating the Celestial North Pole • The Celestial North Pole is currently located near the star • Galactic Equator • Ecliptic • • ISP 205 - Astronomy Gary D. Westfall Lecture 1 13 ISP 205 - Astronomy Gary D. Westfall Early Greek and Roman Cosmology Q The Earth was round The Moon was a sphere The Sun was farther away than the Moon • • The Greeks and Romans thought that the Earth • was the center of the universe and all heavenly objects circled the Earth Q Geocentric ISP 205 - Astronomy Gary D. Westfall • Lecture 1 14 • The Greeks measured the size of the Earth • Eratosthenes noticed that on the first day of summer, and origin of the cosmos • The Greeks and Romans knew Q Lecture 1 Measurements of the Earth • Cosmology is the concept of the basic structure Q Polaris (aptly named!) Locate the constellation Ursa Major, the Big Dipper Locate the outer two stars of the dipper Those 2 stars point at Polaris The distance to Polaris is about 5 times the spacing between the two stars 15 sunlight struck the bottom of a vertical well in Syene at noon To Sun At the same time in Alexandria, at noon June22 the Sun was not directly overhead To zenith but made an angle of 7 degrees at Alexandria To Sun 360 degrees divided by 7 degrees and zenith 7° at Syene is about 50 50 times the distance between Syene Alexandria 7° Syene and Alexandria would be the circumference of the Earth 50 times 5000 stadia is 250,000 stadia ISP 205 - Astronomy Gary D. Westfall Lecture 1 16 Hipparchus Ptolemy • Roman astronomer around 140 AD • Most important contribution was a geometric model of • Roman astronomer, 150 BC • Compiled detailed star catalog • Invented the system of magnitudes to describe the brightness of stars Q Q • • 1 is the brightest, 5 is the dimmest, with each magnitude about a factor 2 dimmer In modern astronomy, each magnitude varies by a factor 2.512 Q • By comparing with previous observations, describing the motions of the planets with superposition of circles Q Precession ISP 205 - Astronomy Gary D. Westfall Lecture 1 17 Epicycles Center of eccentric Earth Equant point Deferent ISP 205 - Astronomy Gary D. Westfall Lecture 1 Usually the planets move east light the moon and sun but occasionally stop and move westward for some time • He invented a complicated mathematical model Hipparchus showed that the Earth’s north pole changes Q the solar system capable of predicting the positions of planets This model lasted more than 1000 years One puzzling observation that he explained was retrograde motion of the planets 19 Epicycles ISP 205 - Astronomy Gary D. Westfall Lecture 1 18