Jupiter was named after the Roman god Zeus. It was discovered in 1609 by Galileo. Jupiter orbits the sun between 471-817 million km away, taking 12 years to revolve while rotating every 9.8 hours.
The document provides information about the dwarf planet Pluto, including details about its eccentric orbit around the sun, composition and surface features, exploration by the New Horizons spacecraft, and its status as the largest object in the Kuiper Belt. Pluto has an eccentric elliptical orbit that takes it from 30 to 39 astronomical units from the sun over 248 Earth years, and it has a surface temperature ranging from -396°F to -378°F with an atmosphere composed primarily of nitrogen. The New Horizons mission launched in 2006 to conduct the first flyby and imaging of Pluto and its largest moon Charon.
If you want to help or donate please donate at my paypal:
dyokimura@gmail.com
information about saturn
SUPPORT ME:
https://www.buymeacoffee.com/dyokimura6
CHECK MY GAMING CHANNEL:
https://www.youtube.com/channel/UCoKOObshfyyxhVkw1VjyQNA
The document discusses facts about Pluto, including that it used to be considered the smallest planet and has at least 3 moons around the same size as itself. Pluto is much colder than Earth without life, orbits the sun in 248 years, and became classified as a dwarf planet in 2006. It was named by an 11-year old girl and is located near Neptune as one of the farthest dwarf planets from the sun, with its 3 moons being named Charon, Hydra and Nix.
Pluto is classified as a dwarf planet located in the Kuiper Belt beyond Neptune's orbit. It has a diameter less than one-fifth of Earth and a surface composed of ice such as methane and nitrogen. Pluto has 5 known moons - Charon, Nix, Hydra, Kerberos, and Styx. In 2015, the New Horizons probe conducted the first flyby of Pluto and provided more details of its geology, moons, and atmosphere.
Pluto is located over 2 billion miles from Earth in space and is too far away to see with the naked eye. It is composed of ice, rock, and craters. Pluto was discovered in the 1930s and has three moons: Nix, Hydra, and Char. A space craft called New Horizons arrived at Pluto in 2015 to learn more about it since scientists cannot observe details of Pluto from Earth. Temperatures on Pluto are extremely cold at -232 Celsius, making it impossible to live there due to the thin atmosphere and weak gravity. A proposed robot would collect dust samples on Pluto to help scientists learn more about its composition through pictures and analysis back on Earth.
Pluto is located over 2 billion miles from Earth in space and is too far away to see with the naked eye. It is composed of ice, rock, and craters. Pluto was discovered in the 1930s and has three moons: Nix, Hydra, and Char. A space craft called New Horizons arrived at Pluto in 2015 to learn more about it since scientists cannot observe details of Pluto from Earth. Temperatures on Pluto are extremely cold at -232 Celsius, making it impossible to live there due to the thin atmosphere and weak gravity. A proposed robot would collect dust samples on Pluto to help scientists learn more about its composition through pictures and analysis back on Earth.
This document provides an overview of exoplanets, including:
- An exoplanet is a planet that orbits a star other than the Sun. Over 1800 exoplanets have been discovered so far.
- The first confirmed detection of an exoplanet was in 1992, though their existence was hypothesized earlier.
- Exoplanet habitability depends on factors like the presence of liquid water, favorable conditions for life, and available energy sources like sunlight or geothermal activity.
The document provides information about the dwarf planet Pluto, including details about its eccentric orbit around the sun, composition and surface features, exploration by the New Horizons spacecraft, and its status as the largest object in the Kuiper Belt. Pluto has an eccentric elliptical orbit that takes it from 30 to 39 astronomical units from the sun over 248 Earth years, and it has a surface temperature ranging from -396°F to -378°F with an atmosphere composed primarily of nitrogen. The New Horizons mission launched in 2006 to conduct the first flyby and imaging of Pluto and its largest moon Charon.
If you want to help or donate please donate at my paypal:
dyokimura@gmail.com
information about saturn
SUPPORT ME:
https://www.buymeacoffee.com/dyokimura6
CHECK MY GAMING CHANNEL:
https://www.youtube.com/channel/UCoKOObshfyyxhVkw1VjyQNA
The document discusses facts about Pluto, including that it used to be considered the smallest planet and has at least 3 moons around the same size as itself. Pluto is much colder than Earth without life, orbits the sun in 248 years, and became classified as a dwarf planet in 2006. It was named by an 11-year old girl and is located near Neptune as one of the farthest dwarf planets from the sun, with its 3 moons being named Charon, Hydra and Nix.
Pluto is classified as a dwarf planet located in the Kuiper Belt beyond Neptune's orbit. It has a diameter less than one-fifth of Earth and a surface composed of ice such as methane and nitrogen. Pluto has 5 known moons - Charon, Nix, Hydra, Kerberos, and Styx. In 2015, the New Horizons probe conducted the first flyby of Pluto and provided more details of its geology, moons, and atmosphere.
Pluto is located over 2 billion miles from Earth in space and is too far away to see with the naked eye. It is composed of ice, rock, and craters. Pluto was discovered in the 1930s and has three moons: Nix, Hydra, and Char. A space craft called New Horizons arrived at Pluto in 2015 to learn more about it since scientists cannot observe details of Pluto from Earth. Temperatures on Pluto are extremely cold at -232 Celsius, making it impossible to live there due to the thin atmosphere and weak gravity. A proposed robot would collect dust samples on Pluto to help scientists learn more about its composition through pictures and analysis back on Earth.
Pluto is located over 2 billion miles from Earth in space and is too far away to see with the naked eye. It is composed of ice, rock, and craters. Pluto was discovered in the 1930s and has three moons: Nix, Hydra, and Char. A space craft called New Horizons arrived at Pluto in 2015 to learn more about it since scientists cannot observe details of Pluto from Earth. Temperatures on Pluto are extremely cold at -232 Celsius, making it impossible to live there due to the thin atmosphere and weak gravity. A proposed robot would collect dust samples on Pluto to help scientists learn more about its composition through pictures and analysis back on Earth.
This document provides an overview of exoplanets, including:
- An exoplanet is a planet that orbits a star other than the Sun. Over 1800 exoplanets have been discovered so far.
- The first confirmed detection of an exoplanet was in 1992, though their existence was hypothesized earlier.
- Exoplanet habitability depends on factors like the presence of liquid water, favorable conditions for life, and available energy sources like sunlight or geothermal activity.
Jupiter is the fifth planet from the Sun. It is oversized compared to Earth, with a diameter of 88,703 miles. Galileo first observed Jupiter's four largest moons orbiting it in 1610. Jupiter is a gas giant with no solid surface, composed primarily of hydrogen and helium. It has a strong magnetic field and is surrounded by rings and over 63 natural moons.
This document discusses exoplanets and the search for extraterrestrial life. It describes how over 1800 exoplanets have been discovered orbiting stars other than the sun. It explains several methods used to detect exoplanets, including direct imaging, the transit method, astrometry, and radial velocity. It also discusses characteristics of potentially habitable exoplanets and provides details about Gliese 667 Cc, one of the most Earth-like exoplanets discovered. The document then reviews the history of exoplanet detection and outlines some of the earliest projects in the search for extraterrestrial intelligence, such as Projects Ozma and Phoenix.
This document provides information on 52 moons of Saturn, including their sizes, orbits, and discoveries. Each moon's entry includes 1-3 sentences on its characteristics and 1-2 sentences on its discovery and naming origin derived from mythology. The moons range greatly in size, from Aegaeon at only 0.6 miles wide to Titan over 3,200 miles wide. They were discovered between 1684 and 2008, mostly by the Cassini spacecraft mission to Saturn starting in 2004. The moons are grouped by location and mythology, such as the Norse and Gallic moon groups named after figures in those traditions.
Project about Pluto for Planetary Geology 2010
I updated some information and pictures on this powerpoint on 10/16/12
http://www.youtube.com/watch?v=HEheh1BH34Q
We are in the middle of one of the most exciting moments in history of Astronomy and maybe of mankind. Any minute we will discover our next home. Learn more about the Exoplanet Revolution in this presentation that includes spectacular pictures.
Pluto is the second closest dwarf planet to the Sun. It has a diameter of 2,372 km and 5 moons. Pluto was discovered in 1930 by Clyde Tombaugh and was reclassified as a dwarf planet in 2006.
An exoplanet is a planet that orbits a star other than the Sun. Nearly 2000 exoplanets have been discovered orbiting other stars by detecting their gravitational influence or observing dimming of the star's light as the planet passes in front. The Kepler space telescope has been instrumental in discovering many new exoplanets using the transit method of detection, including some that may be capable of hosting life such as Gliese 581g. As exoplanet discoveries increase, interest in finding signs of life on other worlds outside our solar system continues to grow.
Nearly 2000 exoplanets have been discovered orbiting stars other than the Sun since 1988, including 490 multiple planetary systems. The youngest exoplanet discovered so far is less than 1 million years old and orbits the star Coku Tau 4, located 420 light-years away. Astronomers detected this planet by observing an enormous hole in the dusty disk surrounding its host star.
This PowerPoint is one small part of the Astronomy Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 3000+ slide PowerPoint roadmap, 12 page bundled homework package, modified homework, detailed answer keys, 8 pages of unit notes for students who may require assistance, follow along worksheets, and many review games. The homework and lesson notes chronologically follow the PowerPoint slideshow. The answer keys and unit notes are great for support professionals. The activities and discussion questions in the slideshow and meaningful. The PowerPoint includes built-in instructions, visuals, and follow up questions. Also included are critical class notes (color coded red), project ideas, video links, and review games. This unit also includes four PowerPoint review games (110+ slides each with Answers), 38+ video links, lab handouts, activity sheets, rubrics, materials list, templates, guides, and much more. Also included is a 190 slide first day of school PowerPoint presentation. Teaching Duration = 5+ weeks. Areas of Focus in the Astronomy Topics Unit: The Solar System and the Sun, Order of the Planets, Our Sun, Life Cycle of a Star, Size of Stars, Solar Eclipse, Lunar Eclipse, The Inner Planets, Mercury, Venus, Earth, Moon, Craters, Tides, Phases of the Moon, Mars and Moons, Rocketry, Asteroid Belt, NEOs, The Torino Scale, The Outer Planets and Gas Giants, Jupiter / Moons, Saturn / Moons, Uranus / Moons, Neptune / Moons, Pluto's Demotion, The Kuiper Belt, Oort Cloud, Comets / Other, Beyond the Solar System, Types of Galaxies, Blackholes, Extrasolar Planets, The Big Bang, Dark Matter, Dark Energy, The Special Theory of Relativity, Hubble Space Telescope, Constellations, Spacetime and much more. If you have any questions please feel free to contact me. Thanks again and best wishes. Sincerely, Ryan Murphy M.Ed www.sciencepowerpoint@gmail.com
When a person become rich and famous, by god grace he starts doing something by which he could help people or the creation of God. Carl Kruse is one such person.
The curiosity to find earth-like planet can be dated to long time ago. But because of the incapability of the available technologies, it was a dream to detect planets beyond our solar system. After the time stated, the space research have taken a new leap and opened a new era of information. The concept of Exoplanet born. It can also be referred to as Extra Solar Planet. Any planet which is not within our solar system is Exoplanet. But an absolute definition is quite complex and problematic. So some of the important characteristics of an Exoplanet is it has to be earth-like environment, it can be giant or terrestrial type
Jupiter has 67 confirmed moons, giving it the largest number of moons orbiting a planet in our solar system. The four largest moons, known as the Galilean moons, were discovered by Galileo Galilei in 1610. These moons are by far the largest objects orbiting Jupiter. Eight of Jupiter's moons have nearly circular prograde orbits that are aligned with Jupiter's equator, while the remaining moons have more eccentric retrograde orbits farther from Jupiter. Jupiter's regular moons are believed to have formed from an early circumplanetary disk, while the irregular moons were likely captured asteroids.
Pulsars are neutron stars that emit beams of light and radiation from their poles, causing them to blink on and off from Earth's perspective. They were discovered in 1967 by Jocelyn Bell. Pulsars, along with stars, nebulas, and comets, are celestial bodies that scientists study to learn more about the nature of stars and probe the universe.
Astronomy - State of the Art - ExoplanetsChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the dramatic discoveries of exoplanets or extra-solar planets are discussed.
The document summarizes key facts about the Milky Way galaxy and the universe:
1) A constellation is a group of stars that appear close together but are not actually physically close. Constellations help people navigate the night sky.
2) A light year is the distance light travels in one year, around 6 trillion miles. The closest star to our solar system, Proxima Centauri, is about 4 light years away.
3) A galaxy is a large group of stars bound together by gravity. Our Milky Way galaxy is a spiral galaxy estimated to contain 200 billion stars.
Hi !
I have made this presentation for you so that you know what is space and what is space technology.The one who will download it will be the one who has got 95% knowledge of space and
FOR MORE KNOWLEDGE JUST EMAIL ME ON THIS EMAIL ADDRESS
workplaceid154@gmail.com
Thanks for your downloading
(please spread this presentation to all schools and all institute so that the students or people can get to know about space)
NOTE:THIS IS MICROSOFT 2013 PRESENTATION)
I WILL UPLOAD LOWER VERSIONS OF THIS FILE
THANKS (MADE BY IRTAZA ZAFAR AND
HASEEB AHMED FROM THE CITY SCHOOL CHENAB CAMPUS FSD
Background
We can search for evidence of past, or even present, life forms within our own solar system, find
evidence of simple life on planets around other stars –- a planet where water could be present has
recently be found –- or even detect an intelligent signal from an alien civilization. The speaker was
a project scientist in the most sensitive search, Project Phoenix, ever undertaken. Sadly, no signals
were detected but a new 10 year search using two of the world’s largest radio telescopes is about
to begin and, during the next decade, a giant radio telescope, the Square Kilometer Array, will have
the sensitivity to detect alien signals from across the galaxy.
Jupiter is the largest planet in our solar system, over twice as massive as all other planets combined. It has a dense core and gaseous outer layers. Jupiter has 67 moons, the four largest being Io, Europa, Ganymede, and Callisto. Gravity on Jupiter is much stronger than Earth, and it has been visited by several spacecraft.
Galaxy Forum Kansas 2014 -- Daniel Webb -- Colonizing Mars and Investigations...ILOAHawaii
This document summarizes presentations about future missions to Mars and investigations by the Cassini and Juno spacecraft. It discusses how various organizations like NASA, SpaceX, and Mars One are planning missions to colonize Mars in the coming decades. This includes rovers exploring the surface, delivering cargo and supplies, and eventually sending crews. The document also provides an overview of Cassini's findings at Saturn like liquid water under the ice of Enceladus and methane seas on Titan. Finally, it outlines the goals of the Juno mission to Jupiter to determine the planet's deep structure and composition.
The document discusses three recent discoveries in space exploration. It describes how astronomers have found evidence of "dark matter" making up half of the universe's missing mass by detecting the brightening of stars caused by dead stars passing in front of them. The document also discusses how Hubble photos revealed the universe may contain many more galaxies than previously estimated, around 50 million galaxies. Finally, it discusses a computer simulation suggesting the early solar system may have originally had five giant planets, with one planet getting ejected during a gravitational disturbance caused by Jupiter's shifting orbit.
John Dahlsen is an Australian environmental artist based in Byron Bay. He began working with found objects like driftwood and plastic debris washed ashore in the 1990s. Dahlsen collects these materials from beaches and arranges them into sculptures and assemblages that bring attention to environmental issues. Some of his most popular works include "Ship Wreck," made from found ship parts off the Australian coast, and "Blue River," crafted from recycled plastic bags. Dahlsen's art uses everyday trash to promote recycling and caring for the environment.
Alan Warren was an Australian artist born in 1919 in Victoria. He studied drawing and painting at the National Gallery of Victoria Art School during 1937-38. During World War 2, he served in the camouflage corps disguising perimeter defenses in Darwin. After the war, he was director of Myer Gallery from 1946-47 and focused on graphic design and painting, particularly still lifes and landscapes. His work was included in several major Australian art surveys and exhibitions. Later in his career, he taught art and managed art galleries while continuing to paint consistently in a semi-abstract style that emphasized geographical contours and pictorial structure with reduced and unmodulated color.
Jupiter is the fifth planet from the Sun. It is oversized compared to Earth, with a diameter of 88,703 miles. Galileo first observed Jupiter's four largest moons orbiting it in 1610. Jupiter is a gas giant with no solid surface, composed primarily of hydrogen and helium. It has a strong magnetic field and is surrounded by rings and over 63 natural moons.
This document discusses exoplanets and the search for extraterrestrial life. It describes how over 1800 exoplanets have been discovered orbiting stars other than the sun. It explains several methods used to detect exoplanets, including direct imaging, the transit method, astrometry, and radial velocity. It also discusses characteristics of potentially habitable exoplanets and provides details about Gliese 667 Cc, one of the most Earth-like exoplanets discovered. The document then reviews the history of exoplanet detection and outlines some of the earliest projects in the search for extraterrestrial intelligence, such as Projects Ozma and Phoenix.
This document provides information on 52 moons of Saturn, including their sizes, orbits, and discoveries. Each moon's entry includes 1-3 sentences on its characteristics and 1-2 sentences on its discovery and naming origin derived from mythology. The moons range greatly in size, from Aegaeon at only 0.6 miles wide to Titan over 3,200 miles wide. They were discovered between 1684 and 2008, mostly by the Cassini spacecraft mission to Saturn starting in 2004. The moons are grouped by location and mythology, such as the Norse and Gallic moon groups named after figures in those traditions.
Project about Pluto for Planetary Geology 2010
I updated some information and pictures on this powerpoint on 10/16/12
http://www.youtube.com/watch?v=HEheh1BH34Q
We are in the middle of one of the most exciting moments in history of Astronomy and maybe of mankind. Any minute we will discover our next home. Learn more about the Exoplanet Revolution in this presentation that includes spectacular pictures.
Pluto is the second closest dwarf planet to the Sun. It has a diameter of 2,372 km and 5 moons. Pluto was discovered in 1930 by Clyde Tombaugh and was reclassified as a dwarf planet in 2006.
An exoplanet is a planet that orbits a star other than the Sun. Nearly 2000 exoplanets have been discovered orbiting other stars by detecting their gravitational influence or observing dimming of the star's light as the planet passes in front. The Kepler space telescope has been instrumental in discovering many new exoplanets using the transit method of detection, including some that may be capable of hosting life such as Gliese 581g. As exoplanet discoveries increase, interest in finding signs of life on other worlds outside our solar system continues to grow.
Nearly 2000 exoplanets have been discovered orbiting stars other than the Sun since 1988, including 490 multiple planetary systems. The youngest exoplanet discovered so far is less than 1 million years old and orbits the star Coku Tau 4, located 420 light-years away. Astronomers detected this planet by observing an enormous hole in the dusty disk surrounding its host star.
This PowerPoint is one small part of the Astronomy Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 3000+ slide PowerPoint roadmap, 12 page bundled homework package, modified homework, detailed answer keys, 8 pages of unit notes for students who may require assistance, follow along worksheets, and many review games. The homework and lesson notes chronologically follow the PowerPoint slideshow. The answer keys and unit notes are great for support professionals. The activities and discussion questions in the slideshow and meaningful. The PowerPoint includes built-in instructions, visuals, and follow up questions. Also included are critical class notes (color coded red), project ideas, video links, and review games. This unit also includes four PowerPoint review games (110+ slides each with Answers), 38+ video links, lab handouts, activity sheets, rubrics, materials list, templates, guides, and much more. Also included is a 190 slide first day of school PowerPoint presentation. Teaching Duration = 5+ weeks. Areas of Focus in the Astronomy Topics Unit: The Solar System and the Sun, Order of the Planets, Our Sun, Life Cycle of a Star, Size of Stars, Solar Eclipse, Lunar Eclipse, The Inner Planets, Mercury, Venus, Earth, Moon, Craters, Tides, Phases of the Moon, Mars and Moons, Rocketry, Asteroid Belt, NEOs, The Torino Scale, The Outer Planets and Gas Giants, Jupiter / Moons, Saturn / Moons, Uranus / Moons, Neptune / Moons, Pluto's Demotion, The Kuiper Belt, Oort Cloud, Comets / Other, Beyond the Solar System, Types of Galaxies, Blackholes, Extrasolar Planets, The Big Bang, Dark Matter, Dark Energy, The Special Theory of Relativity, Hubble Space Telescope, Constellations, Spacetime and much more. If you have any questions please feel free to contact me. Thanks again and best wishes. Sincerely, Ryan Murphy M.Ed www.sciencepowerpoint@gmail.com
When a person become rich and famous, by god grace he starts doing something by which he could help people or the creation of God. Carl Kruse is one such person.
The curiosity to find earth-like planet can be dated to long time ago. But because of the incapability of the available technologies, it was a dream to detect planets beyond our solar system. After the time stated, the space research have taken a new leap and opened a new era of information. The concept of Exoplanet born. It can also be referred to as Extra Solar Planet. Any planet which is not within our solar system is Exoplanet. But an absolute definition is quite complex and problematic. So some of the important characteristics of an Exoplanet is it has to be earth-like environment, it can be giant or terrestrial type
Jupiter has 67 confirmed moons, giving it the largest number of moons orbiting a planet in our solar system. The four largest moons, known as the Galilean moons, were discovered by Galileo Galilei in 1610. These moons are by far the largest objects orbiting Jupiter. Eight of Jupiter's moons have nearly circular prograde orbits that are aligned with Jupiter's equator, while the remaining moons have more eccentric retrograde orbits farther from Jupiter. Jupiter's regular moons are believed to have formed from an early circumplanetary disk, while the irregular moons were likely captured asteroids.
Pulsars are neutron stars that emit beams of light and radiation from their poles, causing them to blink on and off from Earth's perspective. They were discovered in 1967 by Jocelyn Bell. Pulsars, along with stars, nebulas, and comets, are celestial bodies that scientists study to learn more about the nature of stars and probe the universe.
Astronomy - State of the Art - ExoplanetsChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the dramatic discoveries of exoplanets or extra-solar planets are discussed.
The document summarizes key facts about the Milky Way galaxy and the universe:
1) A constellation is a group of stars that appear close together but are not actually physically close. Constellations help people navigate the night sky.
2) A light year is the distance light travels in one year, around 6 trillion miles. The closest star to our solar system, Proxima Centauri, is about 4 light years away.
3) A galaxy is a large group of stars bound together by gravity. Our Milky Way galaxy is a spiral galaxy estimated to contain 200 billion stars.
Hi !
I have made this presentation for you so that you know what is space and what is space technology.The one who will download it will be the one who has got 95% knowledge of space and
FOR MORE KNOWLEDGE JUST EMAIL ME ON THIS EMAIL ADDRESS
workplaceid154@gmail.com
Thanks for your downloading
(please spread this presentation to all schools and all institute so that the students or people can get to know about space)
NOTE:THIS IS MICROSOFT 2013 PRESENTATION)
I WILL UPLOAD LOWER VERSIONS OF THIS FILE
THANKS (MADE BY IRTAZA ZAFAR AND
HASEEB AHMED FROM THE CITY SCHOOL CHENAB CAMPUS FSD
Background
We can search for evidence of past, or even present, life forms within our own solar system, find
evidence of simple life on planets around other stars –- a planet where water could be present has
recently be found –- or even detect an intelligent signal from an alien civilization. The speaker was
a project scientist in the most sensitive search, Project Phoenix, ever undertaken. Sadly, no signals
were detected but a new 10 year search using two of the world’s largest radio telescopes is about
to begin and, during the next decade, a giant radio telescope, the Square Kilometer Array, will have
the sensitivity to detect alien signals from across the galaxy.
Jupiter is the largest planet in our solar system, over twice as massive as all other planets combined. It has a dense core and gaseous outer layers. Jupiter has 67 moons, the four largest being Io, Europa, Ganymede, and Callisto. Gravity on Jupiter is much stronger than Earth, and it has been visited by several spacecraft.
Galaxy Forum Kansas 2014 -- Daniel Webb -- Colonizing Mars and Investigations...ILOAHawaii
This document summarizes presentations about future missions to Mars and investigations by the Cassini and Juno spacecraft. It discusses how various organizations like NASA, SpaceX, and Mars One are planning missions to colonize Mars in the coming decades. This includes rovers exploring the surface, delivering cargo and supplies, and eventually sending crews. The document also provides an overview of Cassini's findings at Saturn like liquid water under the ice of Enceladus and methane seas on Titan. Finally, it outlines the goals of the Juno mission to Jupiter to determine the planet's deep structure and composition.
The document discusses three recent discoveries in space exploration. It describes how astronomers have found evidence of "dark matter" making up half of the universe's missing mass by detecting the brightening of stars caused by dead stars passing in front of them. The document also discusses how Hubble photos revealed the universe may contain many more galaxies than previously estimated, around 50 million galaxies. Finally, it discusses a computer simulation suggesting the early solar system may have originally had five giant planets, with one planet getting ejected during a gravitational disturbance caused by Jupiter's shifting orbit.
John Dahlsen is an Australian environmental artist based in Byron Bay. He began working with found objects like driftwood and plastic debris washed ashore in the 1990s. Dahlsen collects these materials from beaches and arranges them into sculptures and assemblages that bring attention to environmental issues. Some of his most popular works include "Ship Wreck," made from found ship parts off the Australian coast, and "Blue River," crafted from recycled plastic bags. Dahlsen's art uses everyday trash to promote recycling and caring for the environment.
Alan Warren was an Australian artist born in 1919 in Victoria. He studied drawing and painting at the National Gallery of Victoria Art School during 1937-38. During World War 2, he served in the camouflage corps disguising perimeter defenses in Darwin. After the war, he was director of Myer Gallery from 1946-47 and focused on graphic design and painting, particularly still lifes and landscapes. His work was included in several major Australian art surveys and exhibitions. Later in his career, he taught art and managed art galleries while continuing to paint consistently in a semi-abstract style that emphasized geographical contours and pictorial structure with reduced and unmodulated color.
Inspiration: interior ideas for perspective drawingFrank Curkovic
The document provides examples of interior perspective drawings using one-point and two-point perspective techniques. It also showcases interior photographs taken by renowned architectural photographer Julius Shulman, known for popularizing mid-century modern architecture through his work. The photos offer inspiration for creating realistic interior perspective drawings.
Art Appreciation: Drawing & Painting UPDATEDPaige Prater
An introduction to the artistic mediums of drawing and painting based on the textbook "Gateways to Art"(2012). Includes a critical thinking exercise at the end asking students to compare Jan van Eyck's artistic practice with Parisian street artist, JR's 'Inside Out' project.
Linear perspective is a technique used in drawings to depict three-dimensional depth on a two-dimensional surface. It was developed in the 15th century and deals with the orientation and location of shapes in space. Key terms in linear perspective include the horizon line, vertical lines, horizontal lines, orthogonal lines that meet at a vanishing point, and the types of perspective drawings which vary based on the number of vanishing points used.
This lesson teaches two point perspective by having students prepare paper with left and right vanishing points and reference lines, both horizontal and vertical, to provide guidelines for adding details to create their own artwork in two point perspective.
The document discusses one-point perspective in Renaissance art. During this time period, artists became interested in creating the illusion of three-dimensional depth in two-dimensional paintings. They used mathematics and observation to develop the technique of linear perspective, which uses vanishing points and orthogonal lines to trick the eye into seeing depth on a flat surface. One-point perspective involves drawing all lines to converge at a single vanishing point located on the horizon line, creating the illusion of objects receding into the distance.
This document summarizes several 20th century art movements including Impressionism, Fauvism, Cubism, Dadaism, Futurism, Surrealism and Abstract Expressionism. It provides 1-2 sentences on each movement's key characteristics and includes 1-3 representative artworks as examples. The document concludes with a suggested art activity and lists its source.
Let's Integrate MuleSoft RPA, COMPOSER, APM with AWS IDP along with Slackshyamraj55
Discover the seamless integration of RPA (Robotic Process Automation), COMPOSER, and APM with AWS IDP enhanced with Slack notifications. Explore how these technologies converge to streamline workflows, optimize performance, and ensure secure access, all while leveraging the power of AWS IDP and real-time communication via Slack notifications.
Removing Uninteresting Bytes in Software FuzzingAftab Hussain
Imagine a world where software fuzzing, the process of mutating bytes in test seeds to uncover hidden and erroneous program behaviors, becomes faster and more effective. A lot depends on the initial seeds, which can significantly dictate the trajectory of a fuzzing campaign, particularly in terms of how long it takes to uncover interesting behaviour in your code. We introduce DIAR, a technique designed to speedup fuzzing campaigns by pinpointing and eliminating those uninteresting bytes in the seeds. Picture this: instead of wasting valuable resources on meaningless mutations in large, bloated seeds, DIAR removes the unnecessary bytes, streamlining the entire process.
In this work, we equipped AFL, a popular fuzzer, with DIAR and examined two critical Linux libraries -- Libxml's xmllint, a tool for parsing xml documents, and Binutil's readelf, an essential debugging and security analysis command-line tool used to display detailed information about ELF (Executable and Linkable Format). Our preliminary results show that AFL+DIAR does not only discover new paths more quickly but also achieves higher coverage overall. This work thus showcases how starting with lean and optimized seeds can lead to faster, more comprehensive fuzzing campaigns -- and DIAR helps you find such seeds.
- These are slides of the talk given at IEEE International Conference on Software Testing Verification and Validation Workshop, ICSTW 2022.
Things to Consider When Choosing a Website Developer for your Website | FODUUFODUU
Choosing the right website developer is crucial for your business. This article covers essential factors to consider, including experience, portfolio, technical skills, communication, pricing, reputation & reviews, cost and budget considerations and post-launch support. Make an informed decision to ensure your website meets your business goals.
Essentials of Automations: The Art of Triggers and Actions in FMESafe Software
In this second installment of our Essentials of Automations webinar series, we’ll explore the landscape of triggers and actions, guiding you through the nuances of authoring and adapting workspaces for seamless automations. Gain an understanding of the full spectrum of triggers and actions available in FME, empowering you to enhance your workspaces for efficient automation.
We’ll kick things off by showcasing the most commonly used event-based triggers, introducing you to various automation workflows like manual triggers, schedules, directory watchers, and more. Plus, see how these elements play out in real scenarios.
Whether you’re tweaking your current setup or building from the ground up, this session will arm you with the tools and insights needed to transform your FME usage into a powerhouse of productivity. Join us to discover effective strategies that simplify complex processes, enhancing your productivity and transforming your data management practices with FME. Let’s turn complexity into clarity and make your workspaces work wonders!
Ivanti’s Patch Tuesday breakdown goes beyond patching your applications and brings you the intelligence and guidance needed to prioritize where to focus your attention first. Catch early analysis on our Ivanti blog, then join industry expert Chris Goettl for the Patch Tuesday Webinar Event. There we’ll do a deep dive into each of the bulletins and give guidance on the risks associated with the newly-identified vulnerabilities.
Fueling AI with Great Data with Airbyte WebinarZilliz
This talk will focus on how to collect data from a variety of sources, leveraging this data for RAG and other GenAI use cases, and finally charting your course to productionalization.
GraphRAG for Life Science to increase LLM accuracyTomaz Bratanic
GraphRAG for life science domain, where you retriever information from biomedical knowledge graphs using LLMs to increase the accuracy and performance of generated answers
Infrastructure Challenges in Scaling RAG with Custom AI modelsZilliz
Building Retrieval-Augmented Generation (RAG) systems with open-source and custom AI models is a complex task. This talk explores the challenges in productionizing RAG systems, including retrieval performance, response synthesis, and evaluation. We’ll discuss how to leverage open-source models like text embeddings, language models, and custom fine-tuned models to enhance RAG performance. Additionally, we’ll cover how BentoML can help orchestrate and scale these AI components efficiently, ensuring seamless deployment and management of RAG systems in the cloud.
CAKE: Sharing Slices of Confidential Data on BlockchainClaudio Di Ciccio
Presented at the CAiSE 2024 Forum, Intelligent Information Systems, June 6th, Limassol, Cyprus.
Synopsis: Cooperative information systems typically involve various entities in a collaborative process within a distributed environment. Blockchain technology offers a mechanism for automating such processes, even when only partial trust exists among participants. The data stored on the blockchain is replicated across all nodes in the network, ensuring accessibility to all participants. While this aspect facilitates traceability, integrity, and persistence, it poses challenges for adopting public blockchains in enterprise settings due to confidentiality issues. In this paper, we present a software tool named Control Access via Key Encryption (CAKE), designed to ensure data confidentiality in scenarios involving public blockchains. After outlining its core components and functionalities, we showcase the application of CAKE in the context of a real-world cyber-security project within the logistics domain.
Paper: https://doi.org/10.1007/978-3-031-61000-4_16
Monitoring and Managing Anomaly Detection on OpenShift.pdfTosin Akinosho
Monitoring and Managing Anomaly Detection on OpenShift
Overview
Dive into the world of anomaly detection on edge devices with our comprehensive hands-on tutorial. This SlideShare presentation will guide you through the entire process, from data collection and model training to edge deployment and real-time monitoring. Perfect for those looking to implement robust anomaly detection systems on resource-constrained IoT/edge devices.
Key Topics Covered
1. Introduction to Anomaly Detection
- Understand the fundamentals of anomaly detection and its importance in identifying unusual behavior or failures in systems.
2. Understanding Edge (IoT)
- Learn about edge computing and IoT, and how they enable real-time data processing and decision-making at the source.
3. What is ArgoCD?
- Discover ArgoCD, a declarative, GitOps continuous delivery tool for Kubernetes, and its role in deploying applications on edge devices.
4. Deployment Using ArgoCD for Edge Devices
- Step-by-step guide on deploying anomaly detection models on edge devices using ArgoCD.
5. Introduction to Apache Kafka and S3
- Explore Apache Kafka for real-time data streaming and Amazon S3 for scalable storage solutions.
6. Viewing Kafka Messages in the Data Lake
- Learn how to view and analyze Kafka messages stored in a data lake for better insights.
7. What is Prometheus?
- Get to know Prometheus, an open-source monitoring and alerting toolkit, and its application in monitoring edge devices.
8. Monitoring Application Metrics with Prometheus
- Detailed instructions on setting up Prometheus to monitor the performance and health of your anomaly detection system.
9. What is Camel K?
- Introduction to Camel K, a lightweight integration framework built on Apache Camel, designed for Kubernetes.
10. Configuring Camel K Integrations for Data Pipelines
- Learn how to configure Camel K for seamless data pipeline integrations in your anomaly detection workflow.
11. What is a Jupyter Notebook?
- Overview of Jupyter Notebooks, an open-source web application for creating and sharing documents with live code, equations, visualizations, and narrative text.
12. Jupyter Notebooks with Code Examples
- Hands-on examples and code snippets in Jupyter Notebooks to help you implement and test anomaly detection models.
AI 101: An Introduction to the Basics and Impact of Artificial IntelligenceIndexBug
Imagine a world where machines not only perform tasks but also learn, adapt, and make decisions. This is the promise of Artificial Intelligence (AI), a technology that's not just enhancing our lives but revolutionizing entire industries.
In the rapidly evolving landscape of technologies, XML continues to play a vital role in structuring, storing, and transporting data across diverse systems. The recent advancements in artificial intelligence (AI) present new methodologies for enhancing XML development workflows, introducing efficiency, automation, and intelligent capabilities. This presentation will outline the scope and perspective of utilizing AI in XML development. The potential benefits and the possible pitfalls will be highlighted, providing a balanced view of the subject.
We will explore the capabilities of AI in understanding XML markup languages and autonomously creating structured XML content. Additionally, we will examine the capacity of AI to enrich plain text with appropriate XML markup. Practical examples and methodological guidelines will be provided to elucidate how AI can be effectively prompted to interpret and generate accurate XML markup.
Further emphasis will be placed on the role of AI in developing XSLT, or schemas such as XSD and Schematron. We will address the techniques and strategies adopted to create prompts for generating code, explaining code, or refactoring the code, and the results achieved.
The discussion will extend to how AI can be used to transform XML content. In particular, the focus will be on the use of AI XPath extension functions in XSLT, Schematron, Schematron Quick Fixes, or for XML content refactoring.
The presentation aims to deliver a comprehensive overview of AI usage in XML development, providing attendees with the necessary knowledge to make informed decisions. Whether you’re at the early stages of adopting AI or considering integrating it in advanced XML development, this presentation will cover all levels of expertise.
By highlighting the potential advantages and challenges of integrating AI with XML development tools and languages, the presentation seeks to inspire thoughtful conversation around the future of XML development. We’ll not only delve into the technical aspects of AI-powered XML development but also discuss practical implications and possible future directions.
Have you ever been confused by the myriad of choices offered by AWS for hosting a website or an API?
Lambda, Elastic Beanstalk, Lightsail, Amplify, S3 (and more!) can each host websites + APIs. But which one should we choose?
Which one is cheapest? Which one is fastest? Which one will scale to meet our needs?
Join me in this session as we dive into each AWS hosting service to determine which one is best for your scenario and explain why!
HCL Notes und Domino Lizenzkostenreduzierung in der Welt von DLAUpanagenda
Webinar Recording: https://www.panagenda.com/webinars/hcl-notes-und-domino-lizenzkostenreduzierung-in-der-welt-von-dlau/
DLAU und die Lizenzen nach dem CCB- und CCX-Modell sind für viele in der HCL-Community seit letztem Jahr ein heißes Thema. Als Notes- oder Domino-Kunde haben Sie vielleicht mit unerwartet hohen Benutzerzahlen und Lizenzgebühren zu kämpfen. Sie fragen sich vielleicht, wie diese neue Art der Lizenzierung funktioniert und welchen Nutzen sie Ihnen bringt. Vor allem wollen Sie sicherlich Ihr Budget einhalten und Kosten sparen, wo immer möglich. Das verstehen wir und wir möchten Ihnen dabei helfen!
Wir erklären Ihnen, wie Sie häufige Konfigurationsprobleme lösen können, die dazu führen können, dass mehr Benutzer gezählt werden als nötig, und wie Sie überflüssige oder ungenutzte Konten identifizieren und entfernen können, um Geld zu sparen. Es gibt auch einige Ansätze, die zu unnötigen Ausgaben führen können, z. B. wenn ein Personendokument anstelle eines Mail-Ins für geteilte Mailboxen verwendet wird. Wir zeigen Ihnen solche Fälle und deren Lösungen. Und natürlich erklären wir Ihnen das neue Lizenzmodell.
Nehmen Sie an diesem Webinar teil, bei dem HCL-Ambassador Marc Thomas und Gastredner Franz Walder Ihnen diese neue Welt näherbringen. Es vermittelt Ihnen die Tools und das Know-how, um den Überblick zu bewahren. Sie werden in der Lage sein, Ihre Kosten durch eine optimierte Domino-Konfiguration zu reduzieren und auch in Zukunft gering zu halten.
Diese Themen werden behandelt
- Reduzierung der Lizenzkosten durch Auffinden und Beheben von Fehlkonfigurationen und überflüssigen Konten
- Wie funktionieren CCB- und CCX-Lizenzen wirklich?
- Verstehen des DLAU-Tools und wie man es am besten nutzt
- Tipps für häufige Problembereiche, wie z. B. Team-Postfächer, Funktions-/Testbenutzer usw.
- Praxisbeispiele und Best Practices zum sofortigen Umsetzen
Taking AI to the Next Level in Manufacturing.pdfssuserfac0301
Read Taking AI to the Next Level in Manufacturing to gain insights on AI adoption in the manufacturing industry, such as:
1. How quickly AI is being implemented in manufacturing.
2. Which barriers stand in the way of AI adoption.
3. How data quality and governance form the backbone of AI.
4. Organizational processes and structures that may inhibit effective AI adoption.
6. Ideas and approaches to help build your organization's AI strategy.
Unlock the Future of Search with MongoDB Atlas_ Vector Search Unleashed.pdfMalak Abu Hammad
Discover how MongoDB Atlas and vector search technology can revolutionize your application's search capabilities. This comprehensive presentation covers:
* What is Vector Search?
* Importance and benefits of vector search
* Practical use cases across various industries
* Step-by-step implementation guide
* Live demos with code snippets
* Enhancing LLM capabilities with vector search
* Best practices and optimization strategies
Perfect for developers, AI enthusiasts, and tech leaders. Learn how to leverage MongoDB Atlas to deliver highly relevant, context-aware search results, transforming your data retrieval process. Stay ahead in tech innovation and maximize the potential of your applications.
#MongoDB #VectorSearch #AI #SemanticSearch #TechInnovation #DataScience #LLM #MachineLearning #SearchTechnology
2. How Jupiter got its Name
• Jupiter was named after Zeus the
Roman god.
3. Who, How, When, and Where
No one really knows who discovered Jupiter but
the credit of its discovery is given t o Galileo.
It was discovered January 7,1609
4. Distance from the sun
• 5.2 au from the sun
• Minimum: 471 million km
• Maximum: 817 million km
5. Jupiter’s revolution/
Rotation
• Its revolution period is 12 years.
• Its rotation period is 9.8 hours.