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Lesson 3
Lesson 3

... from our Sun. Their work helps us better understand the age of Earth, the solar system, and our universe. Astronomers have to work with large numbers because the distances between planets, stars, and the Sun are vast. The numbers are hard to read, and it is difficult to think about the actual distan ...
View PDF
View PDF

... Some protoplanetary disks may spawn many carbon planets simply because they are especially rich in carbon overall, and planet formation proceeds by a carbon-rich condensation sequence. The planets around the pulsar PSR 1257+12 (Wolszczan & Frail 1992) might have been formed in a carbon-rich nebula c ...
Astronomy - Great Smoky Mountains Institute at Tremont
Astronomy - Great Smoky Mountains Institute at Tremont

... floating around between the planets? (Of course not. As far apart as the planets are from each other, there’s nothing of comparable size between them. Even the Asteroid Belt, between Mars and Jupiter, is so small that it would seem like a collection of dust in this model.) Because the Sun is the big ...
CHAPTER 8 Survey of Solar Systems
CHAPTER 8 Survey of Solar Systems

... When several planets appear near each other in the evening sky, we can see that they lie along a linear band extending away from the Sun (fig. 8.4). The planets appear to lie along a line because their orbits, as well as the Earth’s, all lie in nearly the same plane, as shown in the side view of the ...
chapter 04
chapter 04

... • Nebular theory of solar system formation: Cloud of gas and dust gradually collapsed under its own gravity, spinning faster as it shrank. • Condensation theory says dust grains acted as condensation nuclei, beginning formation of ...
03jan13.ppt - Institute for Astronomy
03jan13.ppt - Institute for Astronomy

... top, once about every 26,000 years. • Precession changes the positions in the sky of the celestial poles and the equinoxes.  Polaris won't always be the north star.  The spring equinox, seen by ancient Greeks in Aries, moves westward and is now in Pisces! ...
The barycentric motion of exoplanet host stars
The barycentric motion of exoplanet host stars

... motion of the star about the system barycentre can be approximated by the linear superposition of the reflex motions due to the Keplerian orbit of each individual planet around that star-planet barycentre. If the planets have periods or close approaches such that they are dynamically interacting, th ...
PSCI1030-CHAP016-The Solar System
PSCI1030-CHAP016-The Solar System

... • Synodic Period – the time interval between two successive conjunctions of the planet with the Sun as observed from earth • Sidereal = P1  P1 = 88 Earth Days • Synodic = P1  P1  P3= 116 Earth Days Copyright © Houghton Mifflin Company. All rights reserved. ...
May - Hawaiian Astronomical Society
May - Hawaiian Astronomical Society

... streaming out to the suspects. The seller went completely quiet for more than 2 weeks, while the tester claimed not to understand my test results. It looked pretty bad for awhile, and then pieces of this puzzling predicament began falling into place. The ad for this mirror stated that it had a chip ...
Chapter 2
Chapter 2

... months. We now know that the event was actually a supernova: the explosion of a giant star, which scattered most of its mass into space (see Chapter 21). It left behind a remnant that is still detectable today, nine centuries later. The Chinese data are a prime source of historical information for s ...
Part A
Part A

... 2. A light-year is a measurement of time. 3. Stars shine because there are nuclear reactions in their cores. 4. Sunspots appear dark because they are cooler than nearby areas. ...
Activity 1 - Galaxies
Activity 1 - Galaxies

... Telescopes can be designed to detect any type of electromagnetic wave. This advance in technology has allowed astronomers to generate images of objects in space from the visible light, infra-red, radio waves, X-rays and any other electromagnetic waves they emit. Astronomers have learnt a great deal ...
Astronomical Coordinates, Distances and Magnitudes
Astronomical Coordinates, Distances and Magnitudes

... Polar Reference Systems (RSs) are the most natural systems to define the position of a point located at an unknown distance. These are natural systems used since childhood to point towards something; the easiest version is to use the ground as a reference plane and mark the location of an object by ...
Longevity of moons around habitable planets
Longevity of moons around habitable planets

... planet in the end. The escaping type requires that the semimajor axis of the moon’s orbit exceed this ratio at some time. A moon can maintain a stable circular orbit inside of 0.36 Hill radii because the perturbation from the Sun is small within this region. Outside of 0.36 Hill radii, the planet ha ...
2011 Solar Walk Media Kit | Contents
2011 Solar Walk Media Kit | Contents

... you get to tour our solar system in luscious 3D graphics. While the app is universal for the iPhone and iPad, the iPad version is breathtaking with crisp graphics and beautiful color. Solar Walk is a nifty astronomy romp from the folks who did the popular Star Walk iPhone and iPad app. Instead of ex ...
EASTERN ARIZONA COLLEGE Lab - Introduction to Astronomy
EASTERN ARIZONA COLLEGE Lab - Introduction to Astronomy

... Identify the phases and visual configurations of the planets and the spatial relationships that create the phases and visual configurations of the planets ...
Option E Sum Pages
Option E Sum Pages

... Apparent motion of stars Daily motion: As the earth rotates in 24 hours the stars seem to rotate while keeping their positions relative to each other. In a direction where an axis can be imagined to go from the south pole to the north pole and onwards one will find the point in the sky which stars s ...
Define the following terms in the space provided
Define the following terms in the space provided

... 3) If astronauts were to travel to the center of the Milky Way galaxy using a spacecraft that travelled at commercial airliner speeds (1,000 km/hour or 278 m/s), how much time would be required to make the journey? The distance from the Earth to the center of the Milky Way is 28,000 ly. Express your ...
THe SCieNCe OF ASTrONOMY
THe SCieNCe OF ASTrONOMY

... we use a solar calendar, meaning a calendar that is synchronized with the seasons so that seasonal events such as the solstices and equinoxes occur on approximately the same dates each year. The origins of our modern solar calendar go back to ancient Egypt, though many details (such as the timing of ...
How far away are the Stars?
How far away are the Stars?

... • First mark position A directly opposite tree. • Move a known distance along the ‘baseline’. • Measure ABC • Deduce unknown distance via trigonometry ...
1 Assignment Discovery Online Curriculum Lesson title
1 Assignment Discovery Online Curriculum Lesson title

... 1. Parallax is the apparent change in position of an object when it's viewed from two different places. Astronomers use this phenomenon to measure the distances to some stars. They assume that the stars are fixed, and as the Earth moves in orbit they take measurements of the apparent shift in positi ...
The Parent Stars of New Extrasolar Planet System Candidates
The Parent Stars of New Extrasolar Planet System Candidates

... it is possible that an inward-migrating planet was accreted by the star, thus changing the stellar surface and explaining the odd abundances observed. Unlike Gliese 876, the two stars HR 810 and HR 7875 are very similar to the sun. They are each close to one solar mass and are slightly younger than ...
6 The gravitational mechanics of the Earth
6 The gravitational mechanics of the Earth

... the orientation of the rotation axes of planets and satellites in the solar system: this plane is called the ecliptic. Most solar system bodies do not move far out of this plane. The Earth's instantaneous rotation or spin is about an axis that is inclined to the ecliptic by about 66j', an algle that ...
earth science
earth science

... 51 On the diagram in your answer booklet, place an X at a location on Earth’s surface where the Sun was directly overhead at some time on December 21. [1] 52 State one factor, other than the tilt of Earth’s axis, that causes seasons to change on Earth. [1] 53 At which latitude is Polaris observed at ...
Ch 11
Ch 11

... Could Jupiter have been a star? • No; it is far too cool and too small for that. It would need to be about 80 times more massive to be even a very faint star ...
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Extraterrestrial life



Extraterrestrial life is life that does not originate from Earth. It is also called alien life, or, if it is a sentient and/or relatively complex individual, an ""extraterrestrial"" or ""alien"" (or, to avoid confusion with the legal sense of ""alien"", a ""space alien""). These as-yet-hypothetical life forms range from simple bacteria-like organisms to beings with civilizations far more advanced than humanity. Although many scientists expect extraterrestrial life to exist, so far no unambiguous evidence for its existence exists.The science of extraterrestrial life is known as exobiology. The science of astrobiology also considers life on Earth as well, and in the broader astronomical context. Meteorites that have fallen to Earth have sometimes been examined for signs of microscopic extraterrestrial life. Since the mid-20th century, there has been an ongoing search for signs of extraterrestrial intelligence, from radios used to detect possible extraterrestrial signals, to telescopes used to search for potentially habitable extrasolar planets. It has also played a major role in works of science fiction. Over the years, science fiction works, especially Hollywood's involvement, has increased the public's interest in the possibility of extraterrestrial life. Some encourage aggressive methods to try to get in contact with life in outer space, whereas others argue that it might be dangerous to actively call attention to Earth.
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