The aim of this quiz is to test your students' knowledge on the Milky Way Galaxy, and revise relevant vocabulary. It contains twenty questions. There is a scoreboard to keep track of points in case you would like to do the quiz as a team game.
The document provides information about the sun and solar system. It describes the key layers of the sun's atmosphere, including the photosphere, chromosphere, and corona. It also classifies and compares the eight planets based on their size, composition, distance from the sun, rotation, and other characteristics. Additionally, it discusses asteroids, comets, and meteors, noting that asteroids reside in the belt between Mars and Jupiter, while comets have elliptical orbits and meteors appear as streaks of light in the night sky.
This document discusses the three main layers of the ocean - the surface layer, thermocline layer, and deep ocean layer. It provides details about each layer: 1) The surface layer or epipelagic zone is mixed by wind and currents, keeping temperatures relatively constant down to around 200m. 2) The thermocline layer lies below and temperatures drop rapidly with depth down to around 1000m, separating the warm surface waters from the cold deep waters. 3) Below the thermocline, the deep ocean layers of bathypelagic, abyssopelagic and hadalpelagic zones have cold, dense waters where temperature and salinity remain uniform with increasing depth.
The Silurian period lasted from approximately 443 to 417 million years ago. During this time, volcanic activity was common and generated lava flows and ash. No new major groups of organisms appeared, though some existing groups flourished. Notable events included the first life emerging on land and the appearance of the earliest vascular plants and insects. The period witnessed the fragmentation of the supercontinent Rodinia and changes in global climate and sea levels.
This presentation provides an overview of ocean topography and the various features of the ocean floor. It describes the continental margin including the continental shelf, slope, and rise. It then explains the abyssal zones and different oceanic divisions like ocean basins, trenches, and seamounts. Key terms are defined such as the Marianas Trench, abyssal plains, and oceanic islands.
Ocean currents are large-scale circulation patterns in the ocean driven by factors like winds, solar heating, and water density differences from temperature and salinity changes. Major current systems include subtropical gyres in each ocean basin characterized by warm equatorial currents, western boundary currents, and eastern return flows. The Antarctic Circumpolar Current is a continuous current that circles Antarctica. Thermohaline circulation involves deep water formation and global overturning. Surface currents redistribute heat globally while deep currents transport nutrients and oxygen. Currents influence climate, marine life distributions, and biogeochemical cycles.
This document provides information on various astronomical tools. It describes different types of telescopes such as refracting telescopes which use lenses and reflecting telescopes which use mirrors. It discusses radio telescopes, space telescopes, and notable space telescopes such as Hubble, Chandra, and Fermi. Space probes, rockets, spaceshuts, rovers, and observatories are also summarized. Important early space missions involving animals and astronauts are mentioned.
Jupiter is the largest planet in our solar system, with a mass more than twice that of all other planets combined. It is composed primarily of gas and liquid and rotates faster than any other planet. Jupiter has the strongest magnetic field of any planet and has over 60 moons, four of which are large moons called the Galilean satellites that were discovered by Galileo. Europa may have subsurface oceans that could potentially support life. Many missions have been sent to Jupiter to study its atmosphere, magnetosphere, rings and moons.
This document provides an overview of several topics in astrophysics, including: 1. It discusses stars and their properties like mass, luminosity, temperature, and the proton-proton chain reaction. 2. It covers neutrinos and their characteristics. 3. It describes neutron stars and their properties, how they are formed in supernovas, and provides some details about Supernova 1987A. 4. It discusses pulsars and their discovery, and properties of neutron stars.
This document discusses shadows, solar eclipses, and lunar eclipses. There are four types of solar eclipses: total, annular, hybrid, and partial. During a total solar eclipse, the moon completely obscures the sun, allowing the solar corona to be seen. An annular solar eclipse occurs when the moon is not large enough to completely cover the sun, leaving a ring of sunlight visible. A hybrid eclipse shifts between total and annular. A partial solar eclipse occurs when the moon only partially obscures the sun. There are also three types of lunar eclipses: total, partial, and penumbral.
The Milky Way Galaxy is a spiral galaxy that contains the solar system and Earth. It is estimated to be 100,000 light years in diameter and contains millions to billions of stars. The galaxy is composed of a disk, halo, and central bulge. Spiral arms in the disk contain dense clouds of gas and dust where new stars are forming. The sun orbits near the edge of the disk at a distance of about 8.2 kiloparsecs from the galactic center. All elements heavier than hydrogen and helium were produced through nuclear fusion in earlier generations of stars within the Milky Way over billions of years.
Star clusters provide insight into stellar evolution. Open clusters contain a few dozen to hundreds of younger, hot stars loosely spaced in a galaxy's disk. Globular clusters contain tens to hundreds of thousands of older, metal-poor stars in a spherical distribution in a galaxy's halo. Measuring a cluster's main-sequence turn-off point allows determining its age. Some globular clusters exhibit evidence of black holes at their centers from observations of white dwarf concentrations.
This document provides information about the layers of Earth's interior. It is divided into three main layers: the crust, mantle, and core. The crust is the outermost layer and is divided into two sublayers - the continental crust (Sima) and oceanic crust (Sial). Sima is less dense and older, while Sial is denser and younger. The mantle, the second layer, is also divided into upper and lower sections. The upper mantle is solid while the lower mantle is molten. The core is the innermost layer and consists of nickel and iron. It has a solid inner core and molten outer core. Temperature and pressure increase significantly with depth into Earth.
Convection currents are caused by the movement of warm materials rising and cool materials sinking. Within the atmosphere, convection is the primary method of heat transfer through the troposphere. Convection also occurs in the mantle as very hot material deep in the mantle rises, cools, sinks, and repeats this cycle. In oceans and pots of water, convection currents form as warmer water rises and cooler water sinks, moving in a continuous cycle. Convection also takes place within the sun as large amounts of hot gas rise towards the surface, cool, and fall back towards the center to repeat the cycle.
There are four main types of galaxies: spiral, elliptical, lenticular, and irregular. Spiral galaxies have a central bulge and rotating spiral arms containing young stars. Elliptical galaxies are spherical and contain mostly older, redder stars. Lenticular galaxies resemble ellipticals but have a disk of gas and dust. Irregular galaxies do not fit into the other categories and often have regions of intense star formation. The Milky Way is classified as a barred spiral galaxy while Andromeda is a spiral galaxy as well.
The document discusses lunar and solar eclipses. It explains that lunar eclipses occur when the Earth passes between the sun and moon, casting its shadow on the moon. Solar eclipses occur when the moon passes between the Earth and sun, casting its shadow on parts of Earth. Eclipses only occur when the sun, Earth, and moon are aligned on the same plane. The document provides details on the conditions required to see each type of eclipse and diagrams demonstrating the geometry of lunar and solar eclipses.