NASA's Mars Exploration Rover mission has involved multiple rovers exploring the surface of Mars since 2003, providing images and analyzing rocks and soil to search for evidence of past water activity. The mission's objectives were to characterize the geology and search for signs of water. Rover findings over the years have included bizarre rock formations thought to be formed by water or impact processes, sand dunes, panoramic views of the landscape, and microscopic images of pebbles showing signs of past water activity.
A short glimpse of geology of the planet Mars. Good for undergraduate and post-graduate students of geology, geography, earth and planetary sciences, astronomy.
Mars is the fourth planet from the Sun and has the largest volcano in the Solar System called Olympus Mons. It has polar ice caps and two small irregular moons named Phobos and Deimos that are likely captured asteroids. While no life has been found, some speculate there could be water or even Martians living on Mars.
This document provides information about Mars, including:
- Mars was once warmer and wetter, with rivers and oceans, but its atmosphere depleted over time.
- Humans would weigh less on Mars due to its lower gravity.
- Robotic missions have explored Mars' surface and found evidence it could have once supported life.
- Mars has volcanoes, canyons, dust storms, and two small moons named Deimos and Phobos.
The Milky Way galaxy contains our solar system. It appears as a dim, glowing band in the night sky where individual stars cannot be distinguished. The halo is a spherical structure surrounding the galaxy with very low star concentration and few gas clouds, containing many globular clusters which are ancient relics from galaxy formation. The Milky Way contains 100-400 billion stars and a disk of gas and dust between the stars. It has a bar-shaped core and spiral arm structure, and consists of a disk of gas, dust, and stars surrounding the core.
NASA has sent multiple spacecraft to Mars to search for evidence of water and potential life. The Viking landers in 1976 tested soil and atmosphere for signs of microbial life. Photos from 1997 showed evidence of flash flooding, and samples from rovers in 2004 indicated past water presence. Curiosity rover findings in 2015 showed aqueous environments, while Opportunity found iron-rich rocks suggesting water circulation. Overall findings point to seasonal water flows leaving dark streaks, and hydrated soil salts with trapped water molecules, suggesting contemporary water forms the streaks. NASA plans to explore these findings further with a 2020 mission.
this is the exploration of mars with everything including videos
the topics are :
-About Mars
-Atmosphere and surface on Mars
-The Largest Volcano on Mars
- The Seasons on Mars
-Mars, the god of War
-The First Rover
-Mars Exploration Rovers
-Future Exploration of Mars
-and videos
NASA's Mars Exploration Rover mission has involved multiple rovers exploring the surface of Mars since 2003, providing images and analyzing rocks and soil to search for evidence of past water activity. The mission's objectives were to characterize the geology and search for signs of water. Rover findings over the years have included bizarre rock formations thought to be formed by water or impact processes, sand dunes, panoramic views of the landscape, and microscopic images of pebbles showing signs of past water activity.
A short glimpse of geology of the planet Mars. Good for undergraduate and post-graduate students of geology, geography, earth and planetary sciences, astronomy.
Mars is the fourth planet from the Sun and has the largest volcano in the Solar System called Olympus Mons. It has polar ice caps and two small irregular moons named Phobos and Deimos that are likely captured asteroids. While no life has been found, some speculate there could be water or even Martians living on Mars.
This document provides information about Mars, including:
- Mars was once warmer and wetter, with rivers and oceans, but its atmosphere depleted over time.
- Humans would weigh less on Mars due to its lower gravity.
- Robotic missions have explored Mars' surface and found evidence it could have once supported life.
- Mars has volcanoes, canyons, dust storms, and two small moons named Deimos and Phobos.
The Milky Way galaxy contains our solar system. It appears as a dim, glowing band in the night sky where individual stars cannot be distinguished. The halo is a spherical structure surrounding the galaxy with very low star concentration and few gas clouds, containing many globular clusters which are ancient relics from galaxy formation. The Milky Way contains 100-400 billion stars and a disk of gas and dust between the stars. It has a bar-shaped core and spiral arm structure, and consists of a disk of gas, dust, and stars surrounding the core.
NASA has sent multiple spacecraft to Mars to search for evidence of water and potential life. The Viking landers in 1976 tested soil and atmosphere for signs of microbial life. Photos from 1997 showed evidence of flash flooding, and samples from rovers in 2004 indicated past water presence. Curiosity rover findings in 2015 showed aqueous environments, while Opportunity found iron-rich rocks suggesting water circulation. Overall findings point to seasonal water flows leaving dark streaks, and hydrated soil salts with trapped water molecules, suggesting contemporary water forms the streaks. NASA plans to explore these findings further with a 2020 mission.
this is the exploration of mars with everything including videos
the topics are :
-About Mars
-Atmosphere and surface on Mars
-The Largest Volcano on Mars
- The Seasons on Mars
-Mars, the god of War
-The First Rover
-Mars Exploration Rovers
-Future Exploration of Mars
-and videos
ORIGIN OF EARTH AND IT’S PLACE IN UNIVERSEShahid Hussain
The document discusses the origin and evolution of the universe, Earth, and life. It describes evidence that supports the Big Bang theory of the origin of the universe approximately 13.8 billion years ago. It explains that galaxies, stars, and planets formed over time through evolutionary processes. The document also discusses different views on the origin and age of the universe, from both religious and scientific perspectives, including the idea of theistic evolution. It provides examples of the immense distances in the universe and compares the age of the Earth and the development of life to timescales in a hypothetical "cosmic calendar" representing the universe's age in one year.
Scientists have been searching for exoplanets, or planets outside our solar system, since the 19th century. The goal is to find a planet that could support life, with factors like liquid water, a suitable atmosphere, and distance from its star to allow temperatures that could support ecosystems. Over 3000 exoplanets have been detected so far using transit and radial velocity methods. As Earth's population and resources are strained, the long term goal is to find another planet that could potentially support human habitation if Earth becomes uninhabitable due to environmental damage or other disasters.
This document discusses active geological processes currently occurring on Mars. While Mars was once volcanically and sedimentarily active on a large scale, it is now considered active only on a small scale due to recent high-resolution imaging. Current small-scale processes include dust storms, dust avalanches, slope streaks caused by dry sand flows, migrating dunes, and recurring slope lineae which may indicate present liquid water. Gullies are formed by seasonal frost or dry ice sublimation and modified over time. Impacts continue to shape the surface by exposing underground ice.
Since Mars was discovered, mankind has been interested in this planet. Many people find that saving humanity depends on the colonization of the Red Planet. Here are 10 interesting facts about the Mars.
The Milky Way galaxy surrounds our solar system and is home to around 200 billion stars including the Sun. It has a spiral shape that is approximately 100,000 light years wide and thick. From certain vantage points near the edge of the Milky Way, the dense concentration of stars can be visible as a thick band of light.
The document provides information about Mars' orbit, rotation, atmosphere and temperature. It then lists past Mars orbiters and landers/rovers. It discusses various geological features of Mars including volcanoes such as Olympus Mons, calderas, lava tubes, rift basins, and Valles Marinaris. Finally, it provides evidence that Mars once had an active hydrologic system through features such as drainage networks, springs, rivers, glaciers and oceans.
This document provides an introduction to the solar system, including planets, the sun, moon, asteroids, meteoroids, and comets. It explains that planets orbit the sun and can be categorized into rocky planets like Earth or gas planets. It also gives some details about the sun, stating that it lies at the heart of the solar system, formed from a cloud of gas and dust around 5 billion years ago, and continues providing light and heat to Earth and the solar system.
The document discusses several active geological processes observed on Mars including slope streaks, gully formation, recurring slope lineae (RSL), dust avalanches, and impacts. Slope streaks are believed to form from downslope movement of dry sand or dust in an almost fluid-like manner, exposing darker material underneath. Gullies are thought to form from seasonal frost or from the sublimation of dry ice blocks, which can slide down dune slopes. RSL are dark flows on steep rocky slopes that are correlated with seasonal frost. Dust avalanches and small asteroid impacts continue to shape Mars' surface and may trigger slope streaks. HiRISE images provide evidence that Mars remains an active planet, with subtle changes
The document discusses facts about planet Earth. It describes Earth's three main layers - the crust, mantle, and core. The crust is made up of tectonic plates that are constantly shifting due to convection currents in the mantle. This movement of the plates over millions of years can cause continents to collide, drift apart, or move past each other in the process of continental drift, which is still occurring today.
This document provides 10 arguments for why the Earth is flat rather than a sphere:
1) The horizon always appears flat regardless of altitude and objects should disappear over a curved horizon.
2) The horizon rises to meet the observer's eye level at all altitudes, which would not occur on a globe.
3) Natural physics dictates that water finds and maintains a level surface, which would not occur on a spinning globe.
4) Spherical trigonometry calculations of surface curvature have not been observed with experiments on standing bodies of water.
Earth is the third planet from the sun and is 12,700km long. It takes one day for Earth to rotate on its axis and one year to revolve around the sun. Earth is nicknamed the blue planet because it is mostly made of water, has gravity, oxygen, plants, animals, and humans, and is the only known living planet.
The inner solar system consists of Mercury, Venus, Earth, and Mars, which are terrestrial planets composed primarily of iron and rock. Earth has one moon while Mars has two small moons. Exploration of the inner solar system has involved numerous spacecraft orbiting and exploring each planet, such as Curiosity and Opportunity rovers on Mars, decades of missions to Venus, and fly-bys and long-term missions to Mercury.
Spiral galaxies consist of a flat, rotating disc containing stars, gas and dust, with a central bulge. Elliptical galaxies are the most common type of galaxy and contain less gas and dust. Irregular galaxies have an irregular, chaotic appearance without distinct structure. Edwin Hubble proved in 1925 that the universe is expanding based on the relationship between galaxy distance and velocity.
The document discusses properties of the Milky Way Galaxy. It is a spiral galaxy containing approximately 200 billion stars. The Sun is located within the galaxy's Orion Arm, about 26,000 light years from the galactic center. Key properties listed include the galaxy's diameter of 90,000 light years and mass of 1 trillion solar masses.
What information from Mars can the astronauts obtain? Describe the condition of the Mars environment. Some scientists discuss the possibility to use greenhouse gas on the atmosphere of planet Mars, to make it habitable. Do you approve of this idea?
The document discusses the search for life in the universe. It summarizes efforts to discover Earth-like exoplanets using techniques like the transit method. The Kepler space telescope aims to discover around 30 Earth-sized planets in habitable zones by monitoring 150,000 stars. The document also discusses techniques to characterize exoplanets, like measuring masses and densities, in order to determine compositions and habitability potentials. It suggests that super-Earths may have stable conditions and geochemistry similar to Earth, making them potentially habitable. The overarching goal is to discover the first Earth-like exoplanets and understand life's diversity and origins from a planetary perspective.
Comet 67P/Churyumov-Gerasimenko is a periodic comet with a 5 by 3 km nucleus that rotates every 12.7 hours. The Rosetta probe arrived at the comet in August 2014, becoming the first spacecraft to orbit a comet. In November 2014, the Philae lander touched down on the comet's surface, and detected organic molecules, providing clues about the early chemistry of our solar system.
The document discusses several key facts about the Earth:
1) Estimates of the Earth's age come from radioactive dating of rocks and minerals, with the oldest being approximately 4.2 billion years old. The Earth formed around 4.5 billion years ago from collisions of planetesimals.
2) Multiple lines of evidence show that the Earth is approximately spherical in shape, including observations of ships disappearing over the horizon and photographs from space. While spherical, the Earth is actually an oblate spheroid due to spinning, being flattened at the poles.
3) Measurements of the positions of stars like Polaris in the northern night sky provide evidence that the Earth must be approximately spherical, as these observations could only
The Solar System an volume of Space defined by the influence of the Sun gravity. It is extra-ordinary complex considered the type and the number of objects that circulate around the Sun. Our knowledge about the Solar System exploded as we started sending spacecrafts at the second half of the twentieth century. This is just a slideshow describing the major objects within the Solar System. 25 Sept 2021
Recent advances in space technology have allowed scientists from different fields to collaborate on studying Near-Earth Objects like comets and asteroids. Both comets and asteroids provide clues about the origins of our solar system. Several asteroids have been discovered to come close to Earth in recent years, including Asteroid 2012 DA14 which had a very close approach in February 2012. Impacts from asteroids and comets have affected Earth in the past and could cause catastrophic effects if a large one collided with Earth, though such collisions are rare.
ORIGIN OF EARTH AND IT’S PLACE IN UNIVERSEShahid Hussain
The document discusses the origin and evolution of the universe, Earth, and life. It describes evidence that supports the Big Bang theory of the origin of the universe approximately 13.8 billion years ago. It explains that galaxies, stars, and planets formed over time through evolutionary processes. The document also discusses different views on the origin and age of the universe, from both religious and scientific perspectives, including the idea of theistic evolution. It provides examples of the immense distances in the universe and compares the age of the Earth and the development of life to timescales in a hypothetical "cosmic calendar" representing the universe's age in one year.
Scientists have been searching for exoplanets, or planets outside our solar system, since the 19th century. The goal is to find a planet that could support life, with factors like liquid water, a suitable atmosphere, and distance from its star to allow temperatures that could support ecosystems. Over 3000 exoplanets have been detected so far using transit and radial velocity methods. As Earth's population and resources are strained, the long term goal is to find another planet that could potentially support human habitation if Earth becomes uninhabitable due to environmental damage or other disasters.
This document discusses active geological processes currently occurring on Mars. While Mars was once volcanically and sedimentarily active on a large scale, it is now considered active only on a small scale due to recent high-resolution imaging. Current small-scale processes include dust storms, dust avalanches, slope streaks caused by dry sand flows, migrating dunes, and recurring slope lineae which may indicate present liquid water. Gullies are formed by seasonal frost or dry ice sublimation and modified over time. Impacts continue to shape the surface by exposing underground ice.
Since Mars was discovered, mankind has been interested in this planet. Many people find that saving humanity depends on the colonization of the Red Planet. Here are 10 interesting facts about the Mars.
The Milky Way galaxy surrounds our solar system and is home to around 200 billion stars including the Sun. It has a spiral shape that is approximately 100,000 light years wide and thick. From certain vantage points near the edge of the Milky Way, the dense concentration of stars can be visible as a thick band of light.
The document provides information about Mars' orbit, rotation, atmosphere and temperature. It then lists past Mars orbiters and landers/rovers. It discusses various geological features of Mars including volcanoes such as Olympus Mons, calderas, lava tubes, rift basins, and Valles Marinaris. Finally, it provides evidence that Mars once had an active hydrologic system through features such as drainage networks, springs, rivers, glaciers and oceans.
This document provides an introduction to the solar system, including planets, the sun, moon, asteroids, meteoroids, and comets. It explains that planets orbit the sun and can be categorized into rocky planets like Earth or gas planets. It also gives some details about the sun, stating that it lies at the heart of the solar system, formed from a cloud of gas and dust around 5 billion years ago, and continues providing light and heat to Earth and the solar system.
The document discusses several active geological processes observed on Mars including slope streaks, gully formation, recurring slope lineae (RSL), dust avalanches, and impacts. Slope streaks are believed to form from downslope movement of dry sand or dust in an almost fluid-like manner, exposing darker material underneath. Gullies are thought to form from seasonal frost or from the sublimation of dry ice blocks, which can slide down dune slopes. RSL are dark flows on steep rocky slopes that are correlated with seasonal frost. Dust avalanches and small asteroid impacts continue to shape Mars' surface and may trigger slope streaks. HiRISE images provide evidence that Mars remains an active planet, with subtle changes
The document discusses facts about planet Earth. It describes Earth's three main layers - the crust, mantle, and core. The crust is made up of tectonic plates that are constantly shifting due to convection currents in the mantle. This movement of the plates over millions of years can cause continents to collide, drift apart, or move past each other in the process of continental drift, which is still occurring today.
This document provides 10 arguments for why the Earth is flat rather than a sphere:
1) The horizon always appears flat regardless of altitude and objects should disappear over a curved horizon.
2) The horizon rises to meet the observer's eye level at all altitudes, which would not occur on a globe.
3) Natural physics dictates that water finds and maintains a level surface, which would not occur on a spinning globe.
4) Spherical trigonometry calculations of surface curvature have not been observed with experiments on standing bodies of water.
Earth is the third planet from the sun and is 12,700km long. It takes one day for Earth to rotate on its axis and one year to revolve around the sun. Earth is nicknamed the blue planet because it is mostly made of water, has gravity, oxygen, plants, animals, and humans, and is the only known living planet.
The inner solar system consists of Mercury, Venus, Earth, and Mars, which are terrestrial planets composed primarily of iron and rock. Earth has one moon while Mars has two small moons. Exploration of the inner solar system has involved numerous spacecraft orbiting and exploring each planet, such as Curiosity and Opportunity rovers on Mars, decades of missions to Venus, and fly-bys and long-term missions to Mercury.
Spiral galaxies consist of a flat, rotating disc containing stars, gas and dust, with a central bulge. Elliptical galaxies are the most common type of galaxy and contain less gas and dust. Irregular galaxies have an irregular, chaotic appearance without distinct structure. Edwin Hubble proved in 1925 that the universe is expanding based on the relationship between galaxy distance and velocity.
The document discusses properties of the Milky Way Galaxy. It is a spiral galaxy containing approximately 200 billion stars. The Sun is located within the galaxy's Orion Arm, about 26,000 light years from the galactic center. Key properties listed include the galaxy's diameter of 90,000 light years and mass of 1 trillion solar masses.
What information from Mars can the astronauts obtain? Describe the condition of the Mars environment. Some scientists discuss the possibility to use greenhouse gas on the atmosphere of planet Mars, to make it habitable. Do you approve of this idea?
The document discusses the search for life in the universe. It summarizes efforts to discover Earth-like exoplanets using techniques like the transit method. The Kepler space telescope aims to discover around 30 Earth-sized planets in habitable zones by monitoring 150,000 stars. The document also discusses techniques to characterize exoplanets, like measuring masses and densities, in order to determine compositions and habitability potentials. It suggests that super-Earths may have stable conditions and geochemistry similar to Earth, making them potentially habitable. The overarching goal is to discover the first Earth-like exoplanets and understand life's diversity and origins from a planetary perspective.
Comet 67P/Churyumov-Gerasimenko is a periodic comet with a 5 by 3 km nucleus that rotates every 12.7 hours. The Rosetta probe arrived at the comet in August 2014, becoming the first spacecraft to orbit a comet. In November 2014, the Philae lander touched down on the comet's surface, and detected organic molecules, providing clues about the early chemistry of our solar system.
The document discusses several key facts about the Earth:
1) Estimates of the Earth's age come from radioactive dating of rocks and minerals, with the oldest being approximately 4.2 billion years old. The Earth formed around 4.5 billion years ago from collisions of planetesimals.
2) Multiple lines of evidence show that the Earth is approximately spherical in shape, including observations of ships disappearing over the horizon and photographs from space. While spherical, the Earth is actually an oblate spheroid due to spinning, being flattened at the poles.
3) Measurements of the positions of stars like Polaris in the northern night sky provide evidence that the Earth must be approximately spherical, as these observations could only
The Solar System an volume of Space defined by the influence of the Sun gravity. It is extra-ordinary complex considered the type and the number of objects that circulate around the Sun. Our knowledge about the Solar System exploded as we started sending spacecrafts at the second half of the twentieth century. This is just a slideshow describing the major objects within the Solar System. 25 Sept 2021
Recent advances in space technology have allowed scientists from different fields to collaborate on studying Near-Earth Objects like comets and asteroids. Both comets and asteroids provide clues about the origins of our solar system. Several asteroids have been discovered to come close to Earth in recent years, including Asteroid 2012 DA14 which had a very close approach in February 2012. Impacts from asteroids and comets have affected Earth in the past and could cause catastrophic effects if a large one collided with Earth, though such collisions are rare.
Recent advances in space technology have allowed scientists from different backgrounds to collaborate on studying Near-Earth Objects like comets and asteroids. Studies of these objects provide clues about the origins of the solar system. Several asteroids have been discovered to come close to Earth in recent years, including Asteroid 2012 DA14 in February 2012. Impacts from asteroids and comets have significantly affected Earth in the past, including possibly causing the extinction of dinosaurs 65 million years ago. On average, objects large enough for an impact are estimated to hit Earth once every 100,000 years or so, with smaller objects hitting more frequently.
The document discusses comets, asteroids, and meteors. It describes comets as icy dirtballs that originate in the outer solar system and develop tails as they warm near the sun. Their tails can stretch for millions of kilometers and are made of dust or ionized gas. Asteroids are rocky fragments left over from the formation of the solar system and most orbit between Mars and Jupiter. Meteors are small rocky particles from asteroids and comets that burn up in Earth's atmosphere, and meteorites are meteors that survive atmospheric entry.
The Moon formed about 4.45 billion years ago from debris ejected when a large object collided with Earth. It has since been shaped primarily by relentless bombardment from impacts. Exploration of the Moon began with telescopic observations in the 1600s and recent robotic missions have revealed much about its geology and origins, but many questions remain unanswered, motivating continued exploration including future human missions.
This document provides information about the planet Saturn. It discusses Saturn's distance from the sun, diameter, temperature, rotation period, number of moons, composition and other key facts. It specifically mentions that Saturn is known for its prominent ring system, which was discovered by Christian Huygens in 1665 and that the Cassini Division, a gap within the rings, is named after Giovani Cassini who discovered it. The rings extend from 6,630 km to 120,700 km from Saturn's equator and are composed primarily of ice particles.
Meteors are rocks that fly through the sky and sometimes produce meteor showers. Comets have a nucleus made of ice and dust surrounded by a coma and tail. Asteroids orbit the sun in a belt between Mars and Jupiter, and are believed to be remnants of larger planetary bodies.
The Sun's diameter is 864,938 miles, almost 10 times larger than Jupiter and about 109 times the size of Earth. Astronomers study the Sun using instruments to analyze variations in light and the Sun's effect on Earth's climate. Sunspots are relatively cool, dark patches that can be over 10 times the diameter of Earth and follow an 11-year cycle, with the current cycle peaking in the middle of 2000.
The document provides information about astronomy and the solar system. It begins by defining astronomy and describing early astronomers like Copernicus and Galileo. It then discusses concepts like the universe, galaxies, and the Milky Way galaxy. The bulk of the document is focused on defining and describing components of the solar system, including the sun, planets like Earth, Venus, and Mercury, and units like light years and astronomical units. It provides details on concepts like planetary orbits, rotations, and transits. The summary concludes with an overview of the key topics covered.
The document provides an overview of the solar system, including the nine planets and their characteristics. It discusses the inner and outer planets, the rocky and gas planets, and their compositions, sizes, temperatures, and features such as rings and moons. It also describes the asteroid belt and provides details on each planet such as mythology connections, exploration missions, physical properties, and recent reclassification of Pluto as a dwarf planet.
The document provides an overview of the solar system, including descriptions of the Sun, eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune), Pluto, and the asteroid belt. It discusses the composition and features of each celestial body, such as Mercury being the smallest planet with possible volcanic activity, Earth being the only known planet that supports life, and Jupiter being the largest planet composed primarily of gas. Spacecraft that have visited and studied these objects are also mentioned.
This document provides an overview of the planets in our solar system, from Mercury to Uranus. It discusses key facts about each planet such as composition, exploration probes, and notable features. For example, it notes that Mercury is the closest planet to the sun and is named after the Roman messenger god. It also summarizes Venus as Earth's sister planet with extreme temperatures and probes that have explored its surface like Magellan 4.
Solar System Education Presentation Template
If you want to buy this presentation template, please visit http://madlis.com
Good design gets out of the way of the content you are sharing. It helps your audience focus on the content itself instead of the design.
But, it's no secret that most people dislike giving presentations. The dread of public speaking consistently ranks among the greatest fears in public surveys.
This presentation slides can help you reduce the anxiety involved with giving a presentation. Well-designed slides not only build your own confidence, they make your key points clearer to the audience.
Solar System Education Presentation Template
If you want to buy this presentation template, please visit http://madlis.com
Good design gets out of the way of the content you are sharing. It helps your audience focus on the content itself instead of the design.
But, it's no secret that most people dislike giving presentations. The dread of public speaking consistently ranks among the greatest fears in public surveys.
This presentation slides can help you reduce the anxiety involved with giving a presentation. Well-designed slides not only build your own confidence, they make your key points clearer to the audience.
This document discusses debris in our solar system and its importance in understanding the origin and evolution of the early solar system. It provides an overview of asteroids, meteorites, comets, and impact craters on Earth. Evidence suggests an asteroid or comet impact was responsible for the extinction of dinosaurs 65 million years ago. The study of solar system debris holds keys to deciphering the history of our solar system.
The Big Bang Theory is the dominant scientific theory that the universe was created approximately 13.8 billion years ago from the explosion of a single point that hurled matter in all directions. After the initial expansion and cooling, the universe continued to expand and cool, forming stars, galaxies, and everything in the observable universe. A black hole is a region of space where gravity is so strong that not even light can escape, while a wormhole is a theoretical connection between two distant points in spacetime. The Milky Way galaxy is home to over 200 billion stars and contains three main components: the halo, bulge, and disk. On July 20, 1969, Neil Armstrong became the first person to walk on the moon, famously saying "That's
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.
The document discusses Saturn, including its composition, atmosphere, temperature, rings, orbit and rotation, natural satellites, mass and density, and important facts. Saturn is composed primarily of hydrogen and helium. Its upper atmosphere contains ammonia crystals and clouds of water or ammonium hydrosulfide lower down. It has a banded atmosphere with some of the fastest winds in the solar system. Saturn is known for its prominent ring system and numerous moons, including Titan.
CHINA’S GEO-ECONOMIC OUTREACH IN CENTRAL ASIAN COUNTRIES AND FUTURE PROSPECTjpsjournal1
The rivalry between prominent international actors for dominance over Central Asia's hydrocarbon
reserves and the ancient silk trade route, along with China's diplomatic endeavours in the area, has been
referred to as the "New Great Game." This research centres on the power struggle, considering
geopolitical, geostrategic, and geoeconomic variables. Topics including trade, political hegemony, oil
politics, and conventional and nontraditional security are all explored and explained by the researcher.
Using Mackinder's Heartland, Spykman Rimland, and Hegemonic Stability theories, examines China's role
in Central Asia. This study adheres to the empirical epistemological method and has taken care of
objectivity. This study analyze primary and secondary research documents critically to elaborate role of
china’s geo economic outreach in central Asian countries and its future prospect. China is thriving in trade,
pipeline politics, and winning states, according to this study, thanks to important instruments like the
Shanghai Cooperation Organisation and the Belt and Road Economic Initiative. According to this study,
China is seeing significant success in commerce, pipeline politics, and gaining influence on other
governments. This success may be attributed to the effective utilisation of key tools such as the Shanghai
Cooperation Organisation and the Belt and Road Economic Initiative.
Embedded machine learning-based road conditions and driving behavior monitoringIJECEIAES
Car accident rates have increased in recent years, resulting in losses in human lives, properties, and other financial costs. An embedded machine learning-based system is developed to address this critical issue. The system can monitor road conditions, detect driving patterns, and identify aggressive driving behaviors. The system is based on neural networks trained on a comprehensive dataset of driving events, driving styles, and road conditions. The system effectively detects potential risks and helps mitigate the frequency and impact of accidents. The primary goal is to ensure the safety of drivers and vehicles. Collecting data involved gathering information on three key road events: normal street and normal drive, speed bumps, circular yellow speed bumps, and three aggressive driving actions: sudden start, sudden stop, and sudden entry. The gathered data is processed and analyzed using a machine learning system designed for limited power and memory devices. The developed system resulted in 91.9% accuracy, 93.6% precision, and 92% recall. The achieved inference time on an Arduino Nano 33 BLE Sense with a 32-bit CPU running at 64 MHz is 34 ms and requires 2.6 kB peak RAM and 139.9 kB program flash memory, making it suitable for resource-constrained embedded systems.
Software Engineering and Project Management - Introduction, Modeling Concepts...Prakhyath Rai
Introduction, Modeling Concepts and Class Modeling: What is Object orientation? What is OO development? OO Themes; Evidence for usefulness of OO development; OO modeling history. Modeling
as Design technique: Modeling, abstraction, The Three models. Class Modeling: Object and Class Concept, Link and associations concepts, Generalization and Inheritance, A sample class model, Navigation of class models, and UML diagrams
Building the Analysis Models: Requirement Analysis, Analysis Model Approaches, Data modeling Concepts, Object Oriented Analysis, Scenario-Based Modeling, Flow-Oriented Modeling, class Based Modeling, Creating a Behavioral Model.
Optimizing Gradle Builds - Gradle DPE Tour Berlin 2024Sinan KOZAK
Sinan from the Delivery Hero mobile infrastructure engineering team shares a deep dive into performance acceleration with Gradle build cache optimizations. Sinan shares their journey into solving complex build-cache problems that affect Gradle builds. By understanding the challenges and solutions found in our journey, we aim to demonstrate the possibilities for faster builds. The case study reveals how overlapping outputs and cache misconfigurations led to significant increases in build times, especially as the project scaled up with numerous modules using Paparazzi tests. The journey from diagnosing to defeating cache issues offers invaluable lessons on maintaining cache integrity without sacrificing functionality.
1. There are close to 200
billion galaxies in the
observable universe, each
comprising billions of stars
orbiting the galaxy’s center
of mass.
These range from dwarf
galaxies with as few as ten
million stars to giant
galaxies with a 100 trillion
stars.
2. Our Sun completes an orbit of
the Milky Way galaxy about
once every 225million years.
The Milky Way is a barred
spiral galaxy, shaped like a
spiral with a bar across its
center
On this orbit, it travels at a
speed of about 220km (140
miles) per second.
3. The word galaxy comes from an ancient
Greek word for milky (as in lactic). They
called the Milky Way a milky circle.
Edwin Hubble, in the 1920s, was first to
confirm that the Milky Way was just one
of many galaxies.
4. primary science objective is to collect the first space-based
measurements of atmospheric carbon dioxide with the precision,
resolution and coverage needed to characterize its sources and sinks
and quantify their variability over the seasonal cycle.
5. After almost 20 years in space, NASA's Cassini spacecraft
begins the final chapter of its remarkable story of
exploration: its Grand Finale.
End of Mission: 15 Sep 2017
6. Juno is named after a
Roman goddess who
could see through
clouds.
Juno is carrying a
plaque inscribed with
some of Galileo’s
writings from 1610
Juno is scheduled
to end its life by
plunging into
Jupiter in 2018.
7. The Great Red Spot is a huge storm on
Jupiter.
It has raged for at least 350 years. It is so
large that three Earths could fit inside it.
8. Jupiter orbits the Sun once every 11.8 Earth
years.
Jupiter’s interior is made of rock, metal, and
hydrogen compounds.
Below Jupiter’s massive atmosphere
(which is made primarily of hydrogen),
there are layers of compressed hydrogen
gas, liquid metallic hydrogen, and a core
of ice, rock, and metals.
Eight spacecraft have visited Jupiter
Pioneer 10 and 11, Voyager 1 and 2,
Galileo, Cassini, Ulysses, and New
Horizons missions. The Juno mission is its
way to Jupiter and will arrive in July
2016. Other future missions may focus
on the Jovian moons Europa, Ganymede,
and Callisto, and their subsurface
oceans.
9. There could be life near
Saturn
Saturn has 62 moons
10. Saturn spins so
quickly on its axis
that the planet
flattens itself out into
an oblate spheroid.