Supernova - Part 2
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The earliest recorded supernova was SN 185 observed by Chinese astronomers in 185 AD. The brightest recorded was SN 1006 described by Chinese and Arab astronomers. The widely observed SN 1054 produced the Crab Nebula. SN 1572 and SN 1604, observed in the Milky Way galaxy, were important because they were used to argue against the Aristotelian view that the universe beyond the planets was immutable. Telescopes have allowed observation of supernovae in other galaxies, such as SN 1885 in the Andromeda Galaxy. Supernovae provide important information on cosmological distances.
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This document provides an overview of the history of astronomy. It discusses early astronomy among ancient cultures like the Chinese, Egyptians, and Babylonians who made early records of celestial objects. It then covers the Golden Age of astronomy centered in Greece where thinkers like Aristotle and Eratosthenes made advances. Key figures who supported the heliocentric model like Copernicus, Kepler, Galileo, and Newton are also summarized along with their major contributions and findings that helped establish our modern understanding of the solar system and universe. The document concludes with sections on constellations and the motion of the Earth.
Discovering the Universe - Gravitiation
1. Nicolaus Copernicus developed the first heliocentric (sun-centered) model of the solar system to explain observations like the retrograde motion of Mars.
2. Tycho Brahe made extremely accurate observations of planetary motions that allowed Johannes Kepler to deduce his three laws of planetary motion, including that planets orbit in ellipses with the sun at one focus.
3. Isaac Newton later formulated his law of universal gravitation and laws of motion, explaining that gravity is what keeps the planets in orbit around the sun and accounting for Kepler's laws of planetary motion.
Unit e space exploration
The document discusses astronomy and the study of space. It describes some key discoveries and models in astronomy's history, including that planetary orbits are elliptical, not circular. It also summarizes ancient and modern views of the structure of the universe, from geocentric to heliocentric models. Additionally, it outlines the life cycles of stars and describes objects in our solar system like planets, asteroids, comets, and eclipses.
Astronomy by victor r
Ancient cultures like the Chinese, Egyptians, and Babylonians began recording the motions of celestial objects like the sun, moon, and planets over 5,000 years ago to track seasons and plan activities. The Golden Age of astronomy from 600 BC to AD 150 centered in Greece, where scientists like Aristotle and Eratosthenes made early attempts to measure the size and distances of astronomical bodies using geometry and trigonometry. Later, Copernicus, Kepler, Galileo and Newton developed the heliocentric model of the solar system and laws of planetary motion through observations and mathematical analysis, overturning the geocentric Ptolemaic model that had dominated for over 1,000 years. Their work established modern astronomy and understanding of
CA 3.08 The Milky Way Universe
The document discusses the history of understanding the Milky Way galaxy. It describes how ancient cultures had different names for the Milky Way. In the 1600s, Galileo first observed the Milky Way through a telescope and realized it was made up of countless stars. In the 1700s, Thomas Wright hypothesized that the Milky Way was a large collection of stars forming a flat disk. Later astronomers like Herschel, Kapteyn, and Shapley made maps of the Milky Way galaxy and helped establish its size and shape, believing it constituted the entire universe until the 1920s.
Mission mans-legacy-on-space
NASA has a long legacy of space exploration including landing rovers on Mars, exploring planets like Jupiter and Saturn, and landing humans on the Moon. Some of NASA's most notable missions include Pioneer 10/11 which were the first to visit Jupiter and Saturn, Voyager 1/2 which made flybys of Jupiter, Saturn, Uranus, and Neptune, and WMAP which provided a more precise estimate of the age and composition of the universe. Other landmark missions include Spirit and Opportunity on Mars, Cassini-Huygens at Saturn, Chandra observing the universe in X-rays, Viking as the first successful Mars lander, and Hubble which has changed our understanding of the cosmos through its iconic images.
Colour atlas of the universe
This document provides a history of astronomy from ancient times through to the modern era. It describes how early civilizations made basic observations and developed calendars based on the stars. The Greeks made major advances by distinguishing planets from fixed stars and proving the Earth is spherical. Copernicus challenged the Earth-centered Ptolemaic model in 1543 by proposing a Sun-centered model, though his ideas faced opposition. Galileo was an early proponent of the Copernican model through telescopic observations. Kepler developed the first two laws of planetary motion based on Tycho Brahe's accurate observations. Newton's Principia in 1687 marked the beginning of modern astronomy by explaining Kepler's laws through gravitation.
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Discover the awe-inspiring Eagle Nebula: A captivating glimpse into the majestic Starry Pillar of Creation.
Milestones in Astronomy
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This article aims to present the contribution of astronomy and, in particular, the James Webb telescope to the advancement of knowledge about the Universe. Astronomy is the study of the Universe that exists beyond Earth's atmosphere. This includes objects that can be seen with the naked eye, such as the Sun, Moon, planets and stars. It also includes celestial bodies that can only be observed with telescopes or other instruments, such as distant galaxies and small particles, and it also includes things we cannot see, such as dark matter and dark energy. The main goal of the James Webb Telescope is to peer into the past, looking back a few hundred thousand years after the Big Bang. One of the James Webb Telescope's key abilities is its ability to look back through time to the beginning of the Universe, observing the first galaxies and stars. The telescope, which is 1.5 million kilometers from Earth, has already spotted the most distant and oldest galaxy found so far. The James Webb Telescope also made the first detection of a “molecule of life”. The James Webb super telescope, with its great discoveries, shows the importance of the telescope by revealing, with unexpected speed, a series of information that can call cosmological theories into question.
Early Astronomical Instruments
- Sundials use the sun's position to tell time and can only be used outdoors during daylight hours without cloud cover. Ancient examples were placed in prominent locations to indicate solstices and equinoxes.
- Stonehenges were used as celestial calendars, burial sites, sacrificial altars, and defensive structures in ancient times.
- Telescopes allow viewing of distant celestial objects like stars, planets, and galaxies. The Hubble Space Telescope is the most advanced telescope currently in use.
History of Astronomy
Astronomy is known as the science of the entire universe beyond the Earth. It includes the Earth’s gross physical properties: its mass and rotation, as they interact with other bodies of the solar system.
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This document provides a history of astronomy from ancient Greece to modern times. It describes how early Greek astronomers like Aristotle and Hipparchus made early observations of celestial objects but believed in a geocentric model where Earth is the center. Ptolemy later created an elaborate geocentric model, though Copernicus, Kepler, and Galileo provided evidence supporting a heliocentric model through observations, Kepler's laws of planetary motion, and Galileo's discoveries with the telescope. Newton later unified physics and astronomy by formulating the law of universal gravitation. Einstein then revolutionized our understanding of motion, space, and time through his theory of relativity.
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An Illustrated Design for Self-Directed 3 D Learning GSTA 2017
The document discusses integrating science, technology, engineering and math (STEM) education through project-based and three-dimensional learning. It provides examples of how various science, technology, engineering and math standards can be combined to form interdisciplinary projects. Students are prompted to work in groups to generate questions that combine ideas from different subject areas into potential real-world problems and solutions involving science, technology, engineering and math concepts as well as literacy and art standards. The goal is to demonstrate how everyday concepts can be used to create robust three-dimensional learning experiences.
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There are several misconceptions about the valence shell of the atom. The key questions that arise in the minds of the learners are:
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