The document discusses a lesson about what killed the dinosaurs. It presents two main explanations - an asteroid impact 65 million years ago, and a supervolcanic eruption. While the asteroid theory is supported by iridium found in rocks from that period, dinosaurs were already declining before the impact. The extinction cleared the way for mammals, and studying fossils helps understand which species were lost and emerged after.
This document provides a history of NASA and its public relations strategies. It discusses key events including the founding of NASA in 1958 in response to the Soviet Union launching Sputnik, the Apollo moon landing missions of the 1960s-70s, and the Space Shuttle program from 1981-2011. The document also examines NASA's public relations challenges during crises like the Apollo 1 and Challenger disasters, and how the agency's PR strategies have evolved from initial secrecy to more open communication and media engagement over time. NASA faces ongoing challenges to gain public support and funding as it works to develop new vehicles and pursue missions to Mars and beyond.
The document examines various hypotheses regarding the origin of life on Earth, such as abiogenesis, the RNA world, and panspermia. It discusses early Earth conditions and the emergence of the earliest life forms. While panspermia provides a favored hypothesis for how life began on our planet, the document concludes that delivery of organic molecules by comets alone was likely not sufficient and that additional triggers were needed to initiate life.
1) The document discusses the discovery and growth of the ozone hole over Antarctica.
2) Research in the 1970s first detected chlorofluorocarbons (CFCs) in the atmosphere, even in very small concentrations, and subsequent research showed that CFCs were destroying ozone molecules in the stratosphere.
3) This led to the realization that human-produced chemicals could be damaging the protective ozone layer and increasing UV radiation exposure worldwide.
The document discusses several theories for the origin of life on Earth, including:
1) Special Creation theory which proposes life was created by God.
2) Spontaneous generation theory which suggests life arose from non-living matter.
3) Biochemical evolution theory (also known as Oparin-Haldane hypothesis) which proposes life emerged from chemical reactions in the early reducing Earth's atmosphere.
4) Recent deep sea hydrothermal vent theory proposes life began near hydrothermal vents on the ocean floor.
1. The document discusses several theories regarding the age of the Earth, including that some scientists believe it is approximately 4.6 billion years old based on evidence from fossils and geology, while some creationists believe it is only around 10,000 years old based on historical documents and some scientific evidence.
2. The document also discusses theories of how life on Earth originated, such as the primordial soup theory that early Earth's atmosphere allowed organic molecules to form, and the endosymbiont theory that early cells incorporated aerobic bacteria in a symbiotic relationship.
3. Determining the age of the Earth and theories of the origin of life involve assumptions and can never be proven absolutely, as scientists with different beliefs
Nobel Prize in Astronomy? Nonsense, you will say, there is no such thing! And you will be right! Today I would like to talk about the Nobel Prizes in Physics awarded for the discoveries directly related to Astronomy. Of course, many scientific advances contributed to the modern understanding of Space. But let’s look at those few that achieved the highest scientific recognition.
The universe began about 14.4 billion years ago.
The Big Bang Theory states that, in the beginning, the universe was all in one place.
To know more, see the presentation.
The document discusses a lesson about what killed the dinosaurs. It presents two main explanations - an asteroid impact 65 million years ago, and a supervolcanic eruption. While the asteroid theory is supported by iridium found in rocks from that period, dinosaurs were already declining before the impact. The extinction cleared the way for mammals, and studying fossils helps understand which species were lost and emerged after.
This document provides a history of NASA and its public relations strategies. It discusses key events including the founding of NASA in 1958 in response to the Soviet Union launching Sputnik, the Apollo moon landing missions of the 1960s-70s, and the Space Shuttle program from 1981-2011. The document also examines NASA's public relations challenges during crises like the Apollo 1 and Challenger disasters, and how the agency's PR strategies have evolved from initial secrecy to more open communication and media engagement over time. NASA faces ongoing challenges to gain public support and funding as it works to develop new vehicles and pursue missions to Mars and beyond.
The document examines various hypotheses regarding the origin of life on Earth, such as abiogenesis, the RNA world, and panspermia. It discusses early Earth conditions and the emergence of the earliest life forms. While panspermia provides a favored hypothesis for how life began on our planet, the document concludes that delivery of organic molecules by comets alone was likely not sufficient and that additional triggers were needed to initiate life.
1) The document discusses the discovery and growth of the ozone hole over Antarctica.
2) Research in the 1970s first detected chlorofluorocarbons (CFCs) in the atmosphere, even in very small concentrations, and subsequent research showed that CFCs were destroying ozone molecules in the stratosphere.
3) This led to the realization that human-produced chemicals could be damaging the protective ozone layer and increasing UV radiation exposure worldwide.
The document discusses several theories for the origin of life on Earth, including:
1) Special Creation theory which proposes life was created by God.
2) Spontaneous generation theory which suggests life arose from non-living matter.
3) Biochemical evolution theory (also known as Oparin-Haldane hypothesis) which proposes life emerged from chemical reactions in the early reducing Earth's atmosphere.
4) Recent deep sea hydrothermal vent theory proposes life began near hydrothermal vents on the ocean floor.
1. The document discusses several theories regarding the age of the Earth, including that some scientists believe it is approximately 4.6 billion years old based on evidence from fossils and geology, while some creationists believe it is only around 10,000 years old based on historical documents and some scientific evidence.
2. The document also discusses theories of how life on Earth originated, such as the primordial soup theory that early Earth's atmosphere allowed organic molecules to form, and the endosymbiont theory that early cells incorporated aerobic bacteria in a symbiotic relationship.
3. Determining the age of the Earth and theories of the origin of life involve assumptions and can never be proven absolutely, as scientists with different beliefs
Nobel Prize in Astronomy? Nonsense, you will say, there is no such thing! And you will be right! Today I would like to talk about the Nobel Prizes in Physics awarded for the discoveries directly related to Astronomy. Of course, many scientific advances contributed to the modern understanding of Space. But let’s look at those few that achieved the highest scientific recognition.
The universe began about 14.4 billion years ago.
The Big Bang Theory states that, in the beginning, the universe was all in one place.
To know more, see the presentation.
Our two-week program, Avasara Young Scientists, was a series of hands-on sessions to raise girls' confidence and skills in STEM (science, technology, engineering and mathematics) subjects through relevant and challenging enquiry activities. You can find a short article about it on Page 2 of this issue of Child Friendly News!
The document discusses the origins and evolution of the universe, Earth, and life. It describes how the Big Bang created the universe approximately 13.7 billion years ago. It then explains how galaxies, stars, and planets formed, including theories about how the solar system originated. The formation and geological history of Earth is covered in detail, breaking its timeline into Precambrian, Paleozoic, Mesozoic, and Cenozoic eras. Key events like the emergence of life and mass extinctions are highlighted.
A study in the journal Science finds evidence of methane being released at specific locations on Mars, indicating ongoing geologic or biological activity on the red planet. This suggests that Mars still has active geological processes, the potential for microbial life under the surface, or both. The discovery of seasonal methane variations further piques scientists' interest in understanding the source and meaning of the gas on Mars.
1) Early life on Earth likely originated between 4-3.5 billion years ago as simple prokaryotic cells without nuclei. 2) Around 2.5 billion years ago, cyanobacteria evolved that could produce oxygen through photosynthesis, gradually changing the atmosphere. 3) Eukaryotic cells with nuclei and organelles like mitochondria and chloroplasts emerged around 1.5 billion years ago through endosymbiotic relationships between bacteria and archaea.
The document summarizes theories about what caused the mass extinction that wiped out the dinosaurs 66 million years ago. The two leading hypotheses are that it was caused by an asteroid impact (the Alvarez hypothesis) or massive volcanic eruptions in India known as the Deccan Traps. Recent evidence has strengthened the asteroid impact theory, finding evidence of an impact crater in the Gulf of Mexico and material from the impact throughout the layers from that time period. However, some scientists argue volcanic activity may have also contributed by weakening ecosystems before the impact. More research is still needed to determine the precise timing and roles of both the asteroid impact and volcanic eruptions.
The document discusses various science and technology related topics that were covered in a quiz or test. It includes questions about the Manhattan Project, the Doomsday Clock, bird vision, the shifting Magnetic North Pole, using lasers to transmit sound, the Curiosity rover taking a selfie, Romeo and Juliet frogs, 3D printing using light projections, manipulating sound to create force fields, how an alcometer works, the redefinition of the kilogram, India's Gaganyaan space mission, Sophia the humanoid receiving a visa, the first AI generated painting sold at auction, Microsoft's underwater data center project that doesn't require cooling, the earliest version of the periodic table, the layers of adhesive tape
This document provides an overview of the history of life on Earth from its beginnings over 4.5 billion years ago to the present. It describes how the early Earth formed and cooled, allowing for the emergence of the first life forms like bacteria in the Precambrian era. The Cambrian explosion saw the first major diversification of multicellular life, including in the seas. Subsequent eras like the Paleozoic, Mesozoic, and Cenozoic witnessed further evolution and radiation of life on land and sea, including plants, insects, dinosaurs, mammals, and eventually humans. Mass extinctions periodically wiped out much life, paving the way for new species to evolve and fill ecological niches.
Diane Guo wrote an essay discussing the costs and ethical issues related to space exploration. Space exploration requires high technology and large financial investments, such as the $109 billion spent on the Apollo program. However, critics argue that the money spent on space could be better used to address problems on Earth like providing clean water and food for those in need. Space exploration can also negatively impact the environment through rocket exhaust and the accumulation of space junk. While it provides some benefits, countries should reduce spending on space and instead focus on developing technologies that directly improve life on Earth.
Utmost scientific fields have redounded from sophisticated proposition at least formerly in recent centuries. Similar changes, or paradigm shifts, rearrange old knowledge in a new frame. Text propositions appear and textbooks available for government textbooks, but you can take a chance on textbooks.
Nuclear energy was discovered through experiments creating the atomic bomb. The first nuclear reactor was created in 1942 at the University of Chicago. Nuclear energy provides a new source of energy through fission or fusion but also poses dangers from radiation. While it has advantages as a clean energy source, nuclear power presents environmental and safety risks such as nuclear waste disposal and potential disasters. There is ongoing debate about the use of nuclear power weighing its benefits against the threats from radiation.
President John F. Kennedy encouraged the space program to send Americans to the moon to achieve preeminence in space for the United States and carry out scientific exploration of the moon. Several uncrewed and crewed Apollo missions tested equipment and modules, with Apollo 11 achieving the first lunar landing in 1969. Tragedy struck in 1967 when a fire during a launch pad test killed three astronauts. Later Apollo missions continued lunar exploration through 1972, including Apollo 13 which had to make an emergency return to Earth after an oxygen tank explosion.
The document discusses the history of determining the age of the Earth. Early estimates ranged from thousands to billions of years based on different methods and assumptions. In the late 19th century, radioactive dating methods were developed that provided evidence the Earth was millions to billions of years old, conflicting with a literal reading of the Bible. This sparked debates around assumptions made in dating methods and their application to estimating the Earth's age. While techniques have improved, disagreement remains on interpreting results within biblical or long-age frameworks.
This is a powerpoint presentation that discusses about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the definition of universe, and some of the theories of the origin of the Universe.
Space research involves scientific studies carried out in outer space using scientific equipment. It covers various disciplines like Earth science, materials science, biology, medicine, and physics. Key developments include the emergence of space research after World War II based on advancing rocket technology, important early satellites like Sputnik 1 and Explorer 1, and establishment of organizations like COSPAR for international cooperation. Major space stations and telescopes like Hubble have significantly advanced space science. Current areas of focus include faster-than-light travel using theoretical warp drives and continued use of the International Space Station for microgravity research.
There is a consensus that the universe has a beginning as well as an end, as the “Big Bang” theory indicates that the universe was dense, hot, and small, and then a big explosion occurred 13.8 billion years ago that expanded this small point in less than a billionth of a second to become It is billions of times larger than its original size in the so-called cosmic inflation phenomenon.
This document summarizes the history of space exploration, beginning with early experiments with rockets and satellites in the 20th century. It discusses key events like the launch of Sputnik 1, the founding of NASA, and the first missions that sent animals (dogs) into space to test the viability of life support systems before human spaceflight. The overall goal of space exploration is discussed - to answer fundamental questions about what exists in space and how resources there could benefit life on Earth, while better understanding our planet and solar system through observation and research beyond our atmosphere.
The document discusses the history and future of space exploration. It outlines key events like Sputnik 1, the first man and woman in space, and the moon landing. Future goals discussed include searching for life on other planets within 20 years, landing humans on Mars by 2023, exploring Jupiter and asteroids, understanding dark matter, and commercial space tourism. It also summarizes India's space agency ISRO and its missions like Chandrayaan and Mars Orbiter Mission. The conclusion reiterates that space continues to be a frontier with many mysteries left to solve.
The document summarizes the history of life on Earth from its beginnings around 4 billion years ago to the present. It describes how life first emerged on Earth through natural chemical and physical processes, with the earliest life forms being microspheres composed of amino acids and RNA. These eventually developed into the first prokaryotic cells through self-replication of their RNA. Further evolution led to eukaryotic cells through endosymbiosis, and complex multicellular organisms developed over time, with major diversifications and several mass extinction events altering life on the planet.
The document summarizes the formation and early history of Earth and life:
1) Around 4.6 billion years ago, Earth formed from a cloud of dust and gas left over from the creation of the Sun.
2) Life first emerged around 3.8-2.5 billion years ago in the form of primitive microbes like cyanobacteria and archea.
3) The first soft-bodied animals appeared around 543 million years ago, marking the end of the Proterozoic Eon and the beginning of complex life on Earth.
The document discusses methods that scientists use to determine the age of the Earth. It explains that radiometric dating is used to measure the decay of radioactive isotopes in rocks and minerals to estimate their age. While this provides a means to directly date some igneous rocks, most rocks cannot be directly dated and must be bracketed between dated materials. The document reviews several examples of dated rocks and materials. Though radiometric dating provides a framework, determining the exact age of the Earth remains an ongoing effort as techniques are refined.
Since NASA launched its Hubble Space Telescope in 1990, space scientists at the University of Arizona in Tucson have used it to expand our knowledge of the Universe time and time again.
1) The document discusses the origin of the universe according to the Big Bang theory. It describes how the universe began as a very small, dense point and has been expanding ever since.
2) The Big Bang theory gained support in 1964 with the discovery of cosmic microwave background radiation by Penzias and Wilson. This provided evidence that the universe had a hot, dense beginning.
3) The theory proposes that nearly 14 billion years ago, the entire visible universe was condensed into a very high density and high temperature condition, and then began rapidly expanding.
Our two-week program, Avasara Young Scientists, was a series of hands-on sessions to raise girls' confidence and skills in STEM (science, technology, engineering and mathematics) subjects through relevant and challenging enquiry activities. You can find a short article about it on Page 2 of this issue of Child Friendly News!
The document discusses the origins and evolution of the universe, Earth, and life. It describes how the Big Bang created the universe approximately 13.7 billion years ago. It then explains how galaxies, stars, and planets formed, including theories about how the solar system originated. The formation and geological history of Earth is covered in detail, breaking its timeline into Precambrian, Paleozoic, Mesozoic, and Cenozoic eras. Key events like the emergence of life and mass extinctions are highlighted.
A study in the journal Science finds evidence of methane being released at specific locations on Mars, indicating ongoing geologic or biological activity on the red planet. This suggests that Mars still has active geological processes, the potential for microbial life under the surface, or both. The discovery of seasonal methane variations further piques scientists' interest in understanding the source and meaning of the gas on Mars.
1) Early life on Earth likely originated between 4-3.5 billion years ago as simple prokaryotic cells without nuclei. 2) Around 2.5 billion years ago, cyanobacteria evolved that could produce oxygen through photosynthesis, gradually changing the atmosphere. 3) Eukaryotic cells with nuclei and organelles like mitochondria and chloroplasts emerged around 1.5 billion years ago through endosymbiotic relationships between bacteria and archaea.
The document summarizes theories about what caused the mass extinction that wiped out the dinosaurs 66 million years ago. The two leading hypotheses are that it was caused by an asteroid impact (the Alvarez hypothesis) or massive volcanic eruptions in India known as the Deccan Traps. Recent evidence has strengthened the asteroid impact theory, finding evidence of an impact crater in the Gulf of Mexico and material from the impact throughout the layers from that time period. However, some scientists argue volcanic activity may have also contributed by weakening ecosystems before the impact. More research is still needed to determine the precise timing and roles of both the asteroid impact and volcanic eruptions.
The document discusses various science and technology related topics that were covered in a quiz or test. It includes questions about the Manhattan Project, the Doomsday Clock, bird vision, the shifting Magnetic North Pole, using lasers to transmit sound, the Curiosity rover taking a selfie, Romeo and Juliet frogs, 3D printing using light projections, manipulating sound to create force fields, how an alcometer works, the redefinition of the kilogram, India's Gaganyaan space mission, Sophia the humanoid receiving a visa, the first AI generated painting sold at auction, Microsoft's underwater data center project that doesn't require cooling, the earliest version of the periodic table, the layers of adhesive tape
This document provides an overview of the history of life on Earth from its beginnings over 4.5 billion years ago to the present. It describes how the early Earth formed and cooled, allowing for the emergence of the first life forms like bacteria in the Precambrian era. The Cambrian explosion saw the first major diversification of multicellular life, including in the seas. Subsequent eras like the Paleozoic, Mesozoic, and Cenozoic witnessed further evolution and radiation of life on land and sea, including plants, insects, dinosaurs, mammals, and eventually humans. Mass extinctions periodically wiped out much life, paving the way for new species to evolve and fill ecological niches.
Diane Guo wrote an essay discussing the costs and ethical issues related to space exploration. Space exploration requires high technology and large financial investments, such as the $109 billion spent on the Apollo program. However, critics argue that the money spent on space could be better used to address problems on Earth like providing clean water and food for those in need. Space exploration can also negatively impact the environment through rocket exhaust and the accumulation of space junk. While it provides some benefits, countries should reduce spending on space and instead focus on developing technologies that directly improve life on Earth.
Utmost scientific fields have redounded from sophisticated proposition at least formerly in recent centuries. Similar changes, or paradigm shifts, rearrange old knowledge in a new frame. Text propositions appear and textbooks available for government textbooks, but you can take a chance on textbooks.
Nuclear energy was discovered through experiments creating the atomic bomb. The first nuclear reactor was created in 1942 at the University of Chicago. Nuclear energy provides a new source of energy through fission or fusion but also poses dangers from radiation. While it has advantages as a clean energy source, nuclear power presents environmental and safety risks such as nuclear waste disposal and potential disasters. There is ongoing debate about the use of nuclear power weighing its benefits against the threats from radiation.
President John F. Kennedy encouraged the space program to send Americans to the moon to achieve preeminence in space for the United States and carry out scientific exploration of the moon. Several uncrewed and crewed Apollo missions tested equipment and modules, with Apollo 11 achieving the first lunar landing in 1969. Tragedy struck in 1967 when a fire during a launch pad test killed three astronauts. Later Apollo missions continued lunar exploration through 1972, including Apollo 13 which had to make an emergency return to Earth after an oxygen tank explosion.
The document discusses the history of determining the age of the Earth. Early estimates ranged from thousands to billions of years based on different methods and assumptions. In the late 19th century, radioactive dating methods were developed that provided evidence the Earth was millions to billions of years old, conflicting with a literal reading of the Bible. This sparked debates around assumptions made in dating methods and their application to estimating the Earth's age. While techniques have improved, disagreement remains on interpreting results within biblical or long-age frameworks.
This is a powerpoint presentation that discusses about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the definition of universe, and some of the theories of the origin of the Universe.
Space research involves scientific studies carried out in outer space using scientific equipment. It covers various disciplines like Earth science, materials science, biology, medicine, and physics. Key developments include the emergence of space research after World War II based on advancing rocket technology, important early satellites like Sputnik 1 and Explorer 1, and establishment of organizations like COSPAR for international cooperation. Major space stations and telescopes like Hubble have significantly advanced space science. Current areas of focus include faster-than-light travel using theoretical warp drives and continued use of the International Space Station for microgravity research.
There is a consensus that the universe has a beginning as well as an end, as the “Big Bang” theory indicates that the universe was dense, hot, and small, and then a big explosion occurred 13.8 billion years ago that expanded this small point in less than a billionth of a second to become It is billions of times larger than its original size in the so-called cosmic inflation phenomenon.
This document summarizes the history of space exploration, beginning with early experiments with rockets and satellites in the 20th century. It discusses key events like the launch of Sputnik 1, the founding of NASA, and the first missions that sent animals (dogs) into space to test the viability of life support systems before human spaceflight. The overall goal of space exploration is discussed - to answer fundamental questions about what exists in space and how resources there could benefit life on Earth, while better understanding our planet and solar system through observation and research beyond our atmosphere.
The document discusses the history and future of space exploration. It outlines key events like Sputnik 1, the first man and woman in space, and the moon landing. Future goals discussed include searching for life on other planets within 20 years, landing humans on Mars by 2023, exploring Jupiter and asteroids, understanding dark matter, and commercial space tourism. It also summarizes India's space agency ISRO and its missions like Chandrayaan and Mars Orbiter Mission. The conclusion reiterates that space continues to be a frontier with many mysteries left to solve.
The document summarizes the history of life on Earth from its beginnings around 4 billion years ago to the present. It describes how life first emerged on Earth through natural chemical and physical processes, with the earliest life forms being microspheres composed of amino acids and RNA. These eventually developed into the first prokaryotic cells through self-replication of their RNA. Further evolution led to eukaryotic cells through endosymbiosis, and complex multicellular organisms developed over time, with major diversifications and several mass extinction events altering life on the planet.
The document summarizes the formation and early history of Earth and life:
1) Around 4.6 billion years ago, Earth formed from a cloud of dust and gas left over from the creation of the Sun.
2) Life first emerged around 3.8-2.5 billion years ago in the form of primitive microbes like cyanobacteria and archea.
3) The first soft-bodied animals appeared around 543 million years ago, marking the end of the Proterozoic Eon and the beginning of complex life on Earth.
The document discusses methods that scientists use to determine the age of the Earth. It explains that radiometric dating is used to measure the decay of radioactive isotopes in rocks and minerals to estimate their age. While this provides a means to directly date some igneous rocks, most rocks cannot be directly dated and must be bracketed between dated materials. The document reviews several examples of dated rocks and materials. Though radiometric dating provides a framework, determining the exact age of the Earth remains an ongoing effort as techniques are refined.
Since NASA launched its Hubble Space Telescope in 1990, space scientists at the University of Arizona in Tucson have used it to expand our knowledge of the Universe time and time again.
1) The document discusses the origin of the universe according to the Big Bang theory. It describes how the universe began as a very small, dense point and has been expanding ever since.
2) The Big Bang theory gained support in 1964 with the discovery of cosmic microwave background radiation by Penzias and Wilson. This provided evidence that the universe had a hot, dense beginning.
3) The theory proposes that nearly 14 billion years ago, the entire visible universe was condensed into a very high density and high temperature condition, and then began rapidly expanding.
The document discusses the early development of artificial satellites from the theoretical work of Konstantin Tsiolkovsky and experimental work of Robert Goddard in the early 20th century. It then summarizes the key events in the launch of early satellites including the Soviet Union's launch of Sputnik 1 in 1957, the first artificial satellite, and the United States' launch of Explorer 1 in 1958. The document concludes that satellites have become an integral part of everyday life and have greatly impacted fields such as communications, navigation, weather monitoring, and more since those early launchings.
Astronomy is the scientific study of celestial objects beyond Earth's atmosphere. It has split into observational and theoretical branches since the 20th century. Nicolaus Copernicus proposed a model with the Sun at the center in the 16th century, though planets still seemed to deviate from perfect circular orbits. Tycho Brahe made precise measurements, which Johannes Kepler used to discover the three laws of planetary motion, including that orbits are elliptical. Modern astronomy began with the Space Age in the 1950s with the launch of Sputnik and the space race between the USSR and US. Major events included Gagarin and Shepard's space flights and the Apollo moon landings. Theories of solar system and galaxy formation continue to be
The document discusses exploring space through electromagnetic waves and telescopes on Earth and in space. It covers early space missions including Sputnik and missions to study planets. Current and future space missions are exploring Mars and building space stations for long term living in space through international cooperation.
Jessica Brothers discusses key technological advancements that have helped expand human knowledge of space. The telescope, introduced by Galileo Galilei in 1609, allowed for magnification of celestial objects. Later telescope designs by Isaac Newton used curved mirrors to gather and reflect light, enabling million-fold magnification. Satellites, first launched by the Soviet Union in 1957, now provide communications, weather monitoring and more. The Space Race between the US and Soviet Union led to major milestones like Sputnik, Yuri Gagarin becoming the first person in space, and the moon landing. Future predicted advances include space colonies in orbit and new spacecraft to further exploration.
The document discusses evidence that supports the Big Bang theory of the origins and evolution of the universe. It describes how observations of distant galaxies provided evidence that the universe is expanding from an initial extremely dense and hot state around 13.7 billion years ago. It also mentions how the cosmic microwave background radiation provides major support for the Big Bang theory and how computer models are used to simulate galaxy formation from the early universe.
Submanyan Chandrasekhar received the 1983 Nobel Prize for calculating the Chandrasekhar limit of 1.4 solar masses, above which a white dwarf will collapse into a neutron star or black hole. Russell Hulse and Joseph Taylor Jr. received the 1993 Prize for discovering the first binary pulsar system, which provided evidence for gravitational waves. Raymond Davis Jr. and Masatoshi Koshiba received half of the 2002 Prize for detecting cosmic neutrinos from the Sun, helping solve the mystery of the missing neutrinos.
NASA was established in 1958 in response to the Soviet Union's launch of Sputnik and the space race of the Cold War era. Its early missions included Project Mercury (1961-1963) which put the first Americans in space, Project Gemini (1965-1966) which practiced space operations like docking and spacewalks, and Project Apollo (1968-1972) which achieved President Kennedy's goal of landing astronauts on the Moon by 1972. NASA's successful Moon landings during Apollo represented one of the largest technological achievements in U.S. history.
The Big Bang theory is the prevailing cosmological model that describes the early development and expansion of the universe, approximately 13.8 billion years ago from an initial extremely hot and dense state. It explains phenomena such as the expansion of space, the abundance of light elements, and the discovery of cosmic microwave background radiation. Evidence for the theory includes measurements of galaxy redshifts and the cosmic microwave background radiation. The theory is widely accepted by the scientific community but still leaves major questions unanswered, such as what caused the initial conditions of the Big Bang.
This document discusses evidence for the possibility of life existing elsewhere in the universe. It first outlines potential habitats for life, including early Earth and extremophiles that can survive in harsh conditions. It then discusses various pieces of evidence found, such as organic molecules in meteorites, methane on Mars, and fossilized microbes in meteorites. However, it also notes limitations, such as the rarity of conditions required to support life as we know it. It concludes by discussing future missions to test the hypothesis of panspermia, such as an experiment to send microorganisms into deep space aboard a Russian spacecraft.
The document discusses recent developments in space exploration and travel. It outlines key milestones such as the first artificial satellites launched by the Soviet Union and the United States in the late 1950s. It also discusses early lunar missions in the 1960s including the first lunar soft landing and the first crewed lunar landing by Apollo 11 in 1969. The document then covers the use of autonomous technologies for deep space exploration and the potential benefits of space exploration including scientific discoveries, economic opportunities, and inspiration.
The document summarizes the timeline of major discoveries in cosmology, including Einstein's theory of general relativity, Hubble's discovery of the expanding universe, and the discovery of the cosmic microwave background radiation by Penzias and Wilson which provided evidence for the Big Bang theory. It then discusses supernovae types and their use in determining the accelerating expansion of the universe, for which three scientists - Perlmutter, Riess, and Schmidt - were awarded the 2011 Nobel Prize in Physics for their findings which suggested the universe is dominated by dark energy.
CHEMATHON- The Science Quiz (Prelims), Resonance '21, St. Stephen's College.Jay Ingle
The Science Quiz, Prelims set of Chemathon, Resonance '21. The set is full of amazing questions. In total there are 20 questions, which are created by Chemistry Undergraduate students of The Chemistry Society, St. Stephen's College. The set will challenge any science student, and students will certainly enjoy the set.
NASA has a long legacy of space exploration including landing rovers on Mars, exploring planets like Jupiter and Saturn, and landing humans on the Moon. Some of NASA's most notable missions include Pioneer 10/11 which were the first to visit Jupiter and Saturn, Voyager 1/2 which made flybys of Jupiter, Saturn, Uranus, and Neptune, and WMAP which provided a more precise estimate of the age and composition of the universe. Other landmark missions include Spirit and Opportunity on Mars, Cassini-Huygens at Saturn, Chandra observing the universe in X-rays, Viking as the first successful Mars lander, and Hubble which has changed our understanding of the cosmos through its iconic images.
As a result of technological development of the second half of the twentieth century, Astronomy suffers big change in its methods that it makes its appearance of observation science to become also a new experimental science, where they appear numerous branches. The advancement of knowledge in Astronomy enabled to establish conjectures about the origin of the Universe that would have arisen through the Big Bang, to identify the existence of a massive black hole in the center of the Milky Way, the discovery of water on Mars, Pluto's demotion to dwarf planet, the existence of exoplanets similar to Earth outside the solar system and the discovery of matter and dark energy in the Universe.
The document summarizes different types of telescopes and space probes used to explore the universe, and some of their key contributions. It discusses radio, infrared, visible light, ultraviolet, X-ray, and gamma ray telescopes, as well as notable space telescopes like Hubble and the upcoming James Webb Space Telescope. It also outlines various space probes sent to study planets, moons, comets and more, providing images to advance scientists' understanding of the solar system. Finally, it lists some technologies that were developed for space exploration but later found applications on Earth.
Scientists have discovered the largest explosion ever observed in the universe. The explosion was detected in the Ophiuchus galaxy cluster located about 390 million light years from Earth. It was caused by a supermassive black hole at the center of a distant galaxy and released five times more energy than the previous largest known cosmological explosion. The blast was powerful enough to punch a cavity in the hot gas surrounding the black hole. It occurred very slowly over hundreds of millions of years. The discovery was made possible through observations using radio, x-ray, and other telescopes, highlighting the importance of multi-wavelength studies to understand highly energetic events in the universe.
Satellites have evolved significantly since Sputnik was launched in 1957. Early satellites were simple devices that gathered basic data and demonstrated orbital technology, while modern satellites can have complex systems and costs over $1 billion. All satellites require power, computers, communication systems, and attitude control to function in space. Though satellites provide important benefits like weather monitoring and GPS, the growing amount of space junk poses risks and may limit future launches if collisions become too dangerous.
Penzias and Wilson discovered a faint 3.5 degree Kelvin microwave background radiation coming from all directions in space. This matched theoretical predictions of radiation leftover from a hot, dense early universe. Princeton astronomers recognized this as evidence supporting the Big Bang theory. The discovery provided strong evidence against the steady state theory of the universe and helped establish the Big Bang as the leading model of cosmic origins.
This document provides a summary of 5 postcards from a US-36 roadtrip from Ohio to Colorado. It describes points of interest along the route such as clay workings in Uhrichsville, Ohio and Zane Shawnee Caverns in Ohio. It also discusses places related to US presidents like Rutherford B. Hayes' birthplace in Delaware, Ohio and sites involving Abraham Lincoln in Illinois. Further locations mentioned include Hannibal, Missouri known for its connection to Mark Twain, and landmarks in Denver, Colorado at the route's end.
This document provides a summary of 5 postcards from a road trip along US Route 35 in 1962. It describes attractions along the route from Michigan City, Indiana to Charleston, West Virginia. Some highlights mentioned include Indiana Dunes State Park in Indiana, attractions in Dayton, Ohio like Carillon Historical Park, and the West Virginia State Capitol building in Charleston. The summary focuses on giving a high-level overview of places visited and sights seen along the 416 mile route across Indiana and Ohio in the early 1960s.
- The document describes the author's memories of attending elementary school in 1962 in Saginaw, Michigan in the 3rd and 4th grades. It discusses daily school life, new schools being built, the banning of school prayer, reading instruction methods, and desegregation issues.
- Key events mentioned include the opening of a new elementary school to relieve overcrowding, the Supreme Court banning school-sponsored prayer in 1962, a debate around "look-say" vs phonetic reading instruction methods, and the challenges of desegregating schools in the North.
- The author provides photos from their class and writing assignments from the time period to illustrate aspects of school in 1962.
This document provides a summary of children's books published in 1962. It begins by introducing the context of staying indoors on a rainy day and imagining reading books from 1962 when the author was a child. The document then lists and describes representative books from different categories of children's books from 1962, including folk tales, fantasies, science books, biographies, and series books. It concludes by discussing the Mary Poppins books and announcing plans to re-read one from 1962.
This document provides a summary of 5 postcards from a road trip along US Route 31 from Michigan to Alabama in 1962. The summary includes:
1) US-31 runs from Mackinaw City, Michigan to Spanish Fort, Alabama, passing through 5 states. Points of interest summarized along the route include sand dunes in Michigan, the Indianapolis Motor Speedway Museum in Indiana, and The Parthenon in Nashville, Tennessee.
2) The route passes near Mammoth Cave National Park in Kentucky, and ends in Mobile, Alabama, where it previously passed under Mobile Bay through the Bankhead Tunnel.
3) The document aims to summarize sights and experiences one might have had along US-31 in 1962
Last Gasp Win for the Celtics - Remembering NBA Finals of 1962Donald Dale Milne
The document summarizes the 1962 NBA Finals between the Boston Celtics and Los Angeles Lakers. It was a tightly contested 7-game series that came down to the final play. In Game 7, with 5 seconds left and tied 100-100, the Lakers missed a shot that would have won them the title. The Celtics went on to win 110-107 in overtime, claiming their sixth championship in a row. The series demonstrated the rivalry between the Celtics dynasty and the rising Lakers in a dramatic 7th game finish.
Roadtrip Highlights Along US-30, the Lincoln HighwayDonald Dale Milne
This document provides a summary of highlights along the Lincoln Highway and US Route 30 traveling from Atlantic City, New Jersey to Astoria, Oregon. Some key points mentioned include:
- US-30 follows the route of the historic Lincoln Highway from Atlantic City to Granger, Wyoming.
- Notable sites along the route include the Franklin Institute in Philadelphia, the Andy Warhol Museum in Pittsburgh, and Palisades-Kepler State Park in Iowa.
- In Oregon, US-30 travels through the scenic Columbia River Gorge before ending at the Astoria Column overlooking the Pacific Ocean in Astoria.
- President John F. Kennedy dedicated the new Dulles International Airport in Virginia, which was the first airport designed specifically for commercial jets.
- The FBI foiled a plot by three Cuban agents to bomb several major department stores in New York City around Thanksgiving using 500 kilos of TNT.
- News headlines also showed progress for the civil rights movement, with the first African Americans elected to various state-level offices in California, Michigan, Massachusetts and Connecticut.
This document summarizes 5 highlights along US Route 29 from Ellicott City, Maryland to Pensacola, Florida. It describes the B&O Railroad Museum in Ellicott City, which opened in 1953. In Washington D.C., it notes the Francis Scott Key Bridge and the Library of Congress. It then discusses Thomas Jefferson's Monticello estate in Charlottesville, Virginia and the Conecuh National Forest in Alabama. The document concludes with the National Naval Aviation Museum in Pensacola, Florida, which first opened in 1963.
Polio, Measles, Influenza, and More – 1962 Had More Problems than a COVID Epi...Donald Dale Milne
We had a lot more virus diseases to worry about in 1962 than COVID! Most viral diseases did not have vaccines yet, and some ravaged the whole world. Read more...
US-28 (US-126) - A Scenic Road Trip through the Cascade RangeDonald Dale Milne
This document provides a summary of a scenic road trip along former US Route 28 and US Route 126 through central Oregon. The 131-mile route travels through the Cascade Mountain range, passing lava tubes, waterfalls, forests, and lakes. Points of interest mentioned include Redmond Caves, Cline Falls State Park, Sisters State Park, McKenzie Pass, Sahalie Falls, and the McKenzie River. The document describes the varied landscape and highlights recreational opportunities along the route.
This document summarizes magazines from 1962 in the United States. There were over 3,250 magazines published with a total circulation of over 311 million. Major general interest magazines included Life, Saturday Evening Post, and Look, which featured photos and articles on current events. Specialty magazines covered many topics from automotive to women's interests. Advertising revenues for magazines totaled $880 million in 1962. The document provides examples and details about the content and audiences of various magazines from 1962.
This document summarizes the history of National Road Trip Day and provides details about a road trip along US Route 27. It discusses how National Road Trip Day originated with Pilot Flying J and falls on the Friday of Memorial Day weekend. It then describes the first cross-country road trip in 1903 from California to New York that helped establish roadtripping. The summary focuses on highlights from the virtual road trip along US-27, including stopping at Hartwick Pines State Park near Grayling, Michigan, known for its old growth white pine trees, and having lunch at Jon's Country Burgers, a drive-in restaurant in Mt. Pleasant, Michigan that has maintained its 1962 atmosphere.
This document summarizes several notable weather events from 1962, including:
- Typhoon Karen devastated Guam in November 1962, destroying thousands of homes and buildings but causing relatively few deaths due to early evacuation warnings.
- Britain experienced its third coldest winter on record from December 1962-January 1963 with heavy snowfall and freezing temperatures that caused over 120,000 deaths.
- A storm in February 1962 caused massive flooding in northern Germany, especially Hamburg, destroying homes and killing over 300 people.
- Several typhoons and tropical storms in Asia caused extensive damage and loss of life, including Typhoon Wanda which killed 434 people in Hong Kong.
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...Sérgio Sacani
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
Describing and Interpreting an Immersive Learning Case with the Immersion Cub...Leonel Morgado
Current descriptions of immersive learning cases are often difficult or impossible to compare. This is due to a myriad of different options on what details to include, which aspects are relevant, and on the descriptive approaches employed. Also, these aspects often combine very specific details with more general guidelines or indicate intents and rationales without clarifying their implementation. In this paper we provide a method to describe immersive learning cases that is structured to enable comparisons, yet flexible enough to allow researchers and practitioners to decide which aspects to include. This method leverages a taxonomy that classifies educational aspects at three levels (uses, practices, and strategies) and then utilizes two frameworks, the Immersive Learning Brain and the Immersion Cube, to enable a structured description and interpretation of immersive learning cases. The method is then demonstrated on a published immersive learning case on training for wind turbine maintenance using virtual reality. Applying the method results in a structured artifact, the Immersive Learning Case Sheet, that tags the case with its proximal uses, practices, and strategies, and refines the free text case description to ensure that matching details are included. This contribution is thus a case description method in support of future comparative research of immersive learning cases. We then discuss how the resulting description and interpretation can be leveraged to change immersion learning cases, by enriching them (considering low-effort changes or additions) or innovating (exploring more challenging avenues of transformation). The method holds significant promise to support better-grounded research in immersive learning.
The debris of the ‘last major merger’ is dynamically youngSérgio Sacani
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Or: Beyond linear.
Abstract: Equivariant neural networks are neural networks that incorporate symmetries. The nonlinear activation functions in these networks result in interesting nonlinear equivariant maps between simple representations, and motivate the key player of this talk: piecewise linear representation theory.
Disclaimer: No one is perfect, so please mind that there might be mistakes and typos.
dtubbenhauer@gmail.com
Corrected slides: dtubbenhauer.com/talks.html
hematic appreciation test is a psychological assessment tool used to measure an individual's appreciation and understanding of specific themes or topics. This test helps to evaluate an individual's ability to connect different ideas and concepts within a given theme, as well as their overall comprehension and interpretation skills. The results of the test can provide valuable insights into an individual's cognitive abilities, creativity, and critical thinking skills
Phenomics assisted breeding in crop improvementIshaGoswami9
As the population is increasing and will reach about 9 billion upto 2050. Also due to climate change, it is difficult to meet the food requirement of such a large population. Facing the challenges presented by resource shortages, climate
change, and increasing global population, crop yield and quality need to be improved in a sustainable way over the coming decades. Genetic improvement by breeding is the best way to increase crop productivity. With the rapid progression of functional
genomics, an increasing number of crop genomes have been sequenced and dozens of genes influencing key agronomic traits have been identified. However, current genome sequence information has not been adequately exploited for understanding
the complex characteristics of multiple gene, owing to a lack of crop phenotypic data. Efficient, automatic, and accurate technologies and platforms that can capture phenotypic data that can
be linked to genomics information for crop improvement at all growth stages have become as important as genotyping. Thus,
high-throughput phenotyping has become the major bottleneck restricting crop breeding. Plant phenomics has been defined as the high-throughput, accurate acquisition and analysis of multi-dimensional phenotypes
during crop growing stages at the organism level, including the cell, tissue, organ, individual plant, plot, and field levels. With the rapid development of novel sensors, imaging technology,
and analysis methods, numerous infrastructure platforms have been developed for phenotyping.
Travis Hills' Endeavors in Minnesota: Fostering Environmental and Economic Pr...Travis Hills MN
Travis Hills of Minnesota developed a method to convert waste into high-value dry fertilizer, significantly enriching soil quality. By providing farmers with a valuable resource derived from waste, Travis Hills helps enhance farm profitability while promoting environmental stewardship. Travis Hills' sustainable practices lead to cost savings and increased revenue for farmers by improving resource efficiency and reducing waste.
Authoring a personal GPT for your research and practice: How we created the Q...Leonel Morgado
Thematic analysis in qualitative research is a time-consuming and systematic task, typically done using teams. Team members must ground their activities on common understandings of the major concepts underlying the thematic analysis, and define criteria for its development. However, conceptual misunderstandings, equivocations, and lack of adherence to criteria are challenges to the quality and speed of this process. Given the distributed and uncertain nature of this process, we wondered if the tasks in thematic analysis could be supported by readily available artificial intelligence chatbots. Our early efforts point to potential benefits: not just saving time in the coding process but better adherence to criteria and grounding, by increasing triangulation between humans and artificial intelligence. This tutorial will provide a description and demonstration of the process we followed, as two academic researchers, to develop a custom ChatGPT to assist with qualitative coding in the thematic data analysis process of immersive learning accounts in a survey of the academic literature: QUAL-E Immersive Learning Thematic Analysis Helper. In the hands-on time, participants will try out QUAL-E and develop their ideas for their own qualitative coding ChatGPT. Participants that have the paid ChatGPT Plus subscription can create a draft of their assistants. The organizers will provide course materials and slide deck that participants will be able to utilize to continue development of their custom GPT. The paid subscription to ChatGPT Plus is not required to participate in this workshop, just for trying out personal GPTs during it.
The technology uses reclaimed CO₂ as the dyeing medium in a closed loop process. When pressurized, CO₂ becomes supercritical (SC-CO₂). In this state CO₂ has a very high solvent power, allowing the dye to dissolve easily.
1. More Science News from 1962
By Donald Dale Milne
https://www.roadtrip62.com/more-science-news-from-1962.htm
This week, Roadtrip-‘62 ™ takes a break from the road and looks at scientific news from our favorite year of 1962. At a high level, science is often
divided into three fields: Formal sciences, Natural sciences, and Social sciences. The Formal sciences include Mathematics, while the Social sciences focus on
human behavior. I’m focusing on the Natural sciences, which are the study of natural phenomena throughout the universe. For convenience, I will try to find a
couple of important 1962 events in each of the following disciplines of Natural science:
Astronomy,
Biology,
Chemistry,
Geology,
Meteorology,
Physics
2. Astronomy
Radio telescope at Green Bank Observatory, West Virginia, in 1962.
(Photo from Green Bank Observatory (see https://greenbankobservatory.org/ ) on Flickr, licensed under Creative Commons Attribution-NonCommercial-
NoDerivs 2.0 Generic License (see https://creativecommons.org/licenses/by-nc-nd/2.0/ ).)
The year 1962 saw the first successes in exploration of our solar system using spacecraft. The first solar observatory, OSO, orbited the sun from 350
miles above it and revealed that solar flares contain both low-energy and high-energy X-rays. NASA also sent a Venus probe, Mariner II. This spacecraft
confirmed that the Earthy is surrounded by a cloud of micrometeorites or dust. It also studied the atmosphere of Venus. Using a carefully designed flight path,
Mariner II passed both the Earthward and Sunward sides of Venus. In addition to the space probes, two new radio antennae went into service on Earth in 1962.
One was at Green Bank, West Virginia and one in Australia. The radio telescope at Green Bank was the largest dish in the world at the time, over 300 feet in
diameter. One 1962 discovery was of radio waves emitted by ever more distant galaxies that were not visible by optical telescopes due to their distance and low
levels of light versus high levels of radio waves. Sadly, the original telescope collapsed in 1988 due to a damaged gusset plate. A new telescope was constructed
on the site and began regular science operations in 2001. The Green Bank location has been the site of radio astronomy telescopes since 1957 and currently
houses seven additional telescopes.
3. Biology
Doctor giving a measles vaccination to a young boy at Fernbank School in Atlanta, Georgia, 1962
(Public domain photo from Centers for Disease Control / Smith Collection.)
As explained on my page "Polio, Measles, Influenza, and More – 1962 Had More Problems than a COVID Epidemic", along with the successful
deployment of the Sabin oral polio vaccine in 1962, other discoveries related to viruses were made (see also https://www.roadtrip62.com/polio-measles-
influenza-and-more-1962-had-more-problems-than-a-COVID-epidemic.htm#polio ). Very small viruses called bacteriophages were discovered that contained
only RNA, but no DNA. Also, a virus that attacks tobacco plants was synthesized in a laboratory, by assembling the proteins needed to create it. Both of these
discoveries were hoped to lead to better virus control in the future. Some viruses that can cause or contribute to cancer were also identified. Their connection to
cancer was not yet well defined however, as they can remain dormant for many years before a cancer may emerge.
4. Chemistry
Technetium sample (Photo by Albert Fenn, from “Matter”, Life Science Library, 1963.)
Researchers working with the so-called “noble” gasses created two compounds of the element xenon. The “noble” gasses were long thought to be
unable to form compounds. However, Dr. Neil Bartlett at the University of British Columbia discovered that the gas platinum hexafluoride oxidized xenon to
form xenon hexafluoroplatinate. Soon after, other researchers at Wheaton College and Argonne National Laboratory created the simpler compound of xenon
tertrafloride. By 1971, more than 80 xenon compounds were known along with many compounds of the other “noble” gasses.
In other elemental research, the element technetium was discovered in trace amounts in a uranium ore sample from South Africa. It had long been
thought to be only manmade and not found in nature. The General Electric Company invented a "direct" process for making diamonds. They were able to create
diamonds directly from carbon using a combination of high pressures and temperatures. Other chemical research was more focused on useful products, such as
developing new detergents that would be more biodegradable than existing detergents. Real soap was highly biodegradable, but modern detergents in 1962 were
not and authorities and the public were becoming concerned about their buildup in the environment and in drinking water sources.
5. Geology
Watch the video of the Project Sedan underground nuclear explosion, Nevada, 1962, at https://www.youtube.com/watch?v=e64T5VEYMYM&t=65s .
In retrospect, one of the most disturbing ideas in geology was under study in 1962. Nuclear tests were moving from the atmosphere to underground
during this year because it was recognized that radioactive fallout in the atmosphere was dangerous worldwide. But the move to underground tests had scientists
and engineers considering purposefully using nuclear blasts to excavate on a large scale. They also considered using the blasts to frack rocks to release oil and
natural gas, and even consolidate loose soils to provide more stable building sites! Tests and studies for such construction projects were carried out under the
name Project Plowshare in the United States and Peaceful Nuclear Explosions in Russia. Project Plowshare began with the Project Gnome test near Carlsbad,
New Mexico in December of 1961. The largest test, Project Sedan, was performed at the Atomic Energy Commission's Yucca Flats Nevada Test Site on July 6,
1962. Another 26 tests were carried out between 1962 and 1973 and resulted in design of one project that almost went to the construction stage. Project Chariot
would have used several hydrogen bombs to excavate an artificial harbor at Cape Thompson, Alaska. It was never carried out due to concerns for native
populations and little potential use for the harbor to justify the risk and expense.
6. Meteorology
TIROS VI weather satellite (Public domain photo by NASA / Glenn Research Center.)
The big news in 1962 was the beginning of the use of satellites for meteorological study and observation. Three TIROS satellites were launched that
year, supplementing the three launched in 1960-1961. Unfortunately, these early satellites were short lived, with all but one failing within a year of launch.
However, they proved the concept of using images from Earth orbit to view the weather and began to make predictions more accurate. They created still pictures
stored on tape as they orbited, that were stored and transmitted back to Earth as the satellite approached a ground command point. After transmission, the tape
was erased or cleaned and readied for more recording. The photos proved particularly useful for analysis of weather in remote areas, including hurricane
analysis, and for decision-making in manned space flights.
7. Physics
Laser retroreflector deployed by Astronaut Buzz Aldrin near the lunar module, 1969. (Public domain photo by NASA.)
Nearly all new discoveries in physics in 1962 were on the subatomic level. For example, two kinds of neutrinos were confirmed, which only raised
more theoretical questions about them and their relations to muons and electrons. All are involved in a certain type of radioactive decay known as beta decay,
and thus are important to the ability to properly calculate what happens during that decay. Many of the experiments on subatomic particles had been carried out
at the University of California at Berkely and the Europen Center for Nuclear Research, but in 1962 a new particle accelerator came online. The Cambridge
Electron accelerator, operated by Harvard University and M.I.T. was the first to push electrons up to the multibillion electron volt energy range. One of the
projects this machine will work on is as an electron microscope to study the internal structure of atoms.
Laser technology continued to improve in 1962 also, with experiments discovering that harmonics could be produced in laser light, just as they occur
with sound. On May 9, in 1962, a red light laser beam was sent through the University of Michigan's 37-inch telescope by a team of scientists from M.I.T. The
beam successfully bounced off the Aristarchus crater on the moon, chosen because of the crater’s high reflectivity, similar to white sand. It was the first lunar
laser ranging experiment. A permanent laser reflector was later set up on the moon during the Apollo 11 landing at Tranquility Base in 1969.
8. The Labs Septic, a hypersurface discovered by Oliver Labs
(Licensed under a Attribution-NonCommercial-ShareAlike 3.0 Unported License (see https://creativecommons.org/licenses/by-nc-sa/3.0/ ).)
I’ll close with a piece of news on mathematics, which is not usually considered one of the Natural Sciences. John Milnor of Princeton University was
awarded the Fields Medal in 1962 for his work in differential topology. The Fields Medal is awarded every four years for outstanding or seminal research in
mathematics. We won’t be considering anything as complex as the complex hypersurface above, but join me anyway next time on Roadtrip-‘62 ™.
9. Visit ROADTRIP-'62 ™ ( https://www.roadtrip62.com/index.htm )for more articles.
Or visit us on Facebook https://www.facebook.com/pages/Roadtrip62/119235794845685 ,
Pinterest https://www.pinterest.com/roadtrip62/ ,
or Flickr https://www.flickr.com/photos/67972937@N07/page1 .
Author of Roadtrip-'62TM ( https://www.roadtrip62.com/ ), Donald Dale Milne
If you haven’t heard of nor Roadtrip-'62 ™ , my name is Don Milne and I'll be your travel guide on this virtual tour of the U. S. of A. First, I suppose
you're wondering why nor Roadtrip-'62 ™ is different from other travel sites? There's a very simple answer: everybody else travels only in space, but we also
travel in time! That's right, we don't just go somewhere, we also go somewhen. And the when is 1962. We'll try to see what's left today from 1962, by driving as
if it were 1962. We will drive on highways as they were in 1962, try to eat only at restaurants that existed in 1962, try to stay only at motels that existed in 1962,
try to buy gas and sundries, play the music, see only the sites across America, and just generally live in America as it was in 1962!
What we will do is enjoy the FUN of cross-country driving. And the fun of cross-country travel is all the differences from our everyday life! We'll talk
about politics, food, great inventions, how people lived, television, and more. We'll get to see some of the people that made our history; that made this country
great. We'll stumble across unexpected pleasures, like one trip I made through Cherokee, North Carolina where I just happened to be in town as the 1996
Olympic Torch procession came through on it's way to Atlanta, Georgia. You really never know what you'll find when you travel!
10. 1962-style US-23 signs
Now, let's see where we'll be going! We're going to drive the US-numbered routes of 1962. Because we'll be using the roads of 1962, that means we
won't be on freeways very much. There weren't many freeways in 1962, as the country had just begun building the Interstate system,, so we'll travel mostly the
two-lanes through every little town on the way. Sometimes even where there was a freeway, I'll go back on the old road just to see what was there. Anyway, even
if there was a freeway in 1962, it was only there for a couple of years and things had not changed much. Sometimes a "business route" ran through a town on the
old route, because there were no services at the freeway interchanges yet.
Just in case you're asking why 1962, it's because I remember 1962. I traveled on my first freeway as a boy with my dad about that time, and fell in love with both
travel and freeways. But, besides my own memories and the fact that it was a time largely before interstate freeways, 1962 is just cool...wait and see! And I'm
writing this virtual tour just because I like to drive. I like to go places, see things, and just drive for the joy of driving! I decided I want to talk about it, to share
the fun with others. I'll be doing the driving on our Roadtrip-'62 ™, but if you see anything you like, I encourage you to get out on the road and enjoy it in person.
This virtual roadtrip may be fun, but there's nothing like the real thing!