1. Bubba and Robbi plan to travel to Mars to build and test an inflatable habitat called "Bubble Technology".
2. The bubble concept involves a self-transporting inflatable rover that expands into a shelter once a suitable location is found. Prefabricated materials from Earth are combined with in situ resource utilization, like filling structural voids with sintered Martian sand.
3. The document discusses construction methods like inflating successive layers and filling voids to form support pillars and a protective sintered brick dome. Locating the bubble in Valles Marineris is proposed to take advantage of thicker atmosphere and potential water sources.
A volcano is a vent in the Earth's surface that allows magma, lava, gases, and pieces of rock to erupt out. Volcanoes occur near the boundaries of the Earth's tectonic plates as they push together or pull apart. They can be active and currently erupting, dormant if not erupting recently but capable of future eruptions, or extinct if no future eruptions are expected.
This document provides an overview of impact cratering mechanics and morphology. It explains that when objects impact planetary surfaces, they release enormous amounts of kinetic energy that excavates craters. There are two main types of craters - simple bowl-shaped craters and more complex craters with interior structures like terraces and central peaks. The size and morphology of craters depends on factors like the impacting object's energy, the planet's gravity, and the properties of the surface materials. Heavily cratered surfaces on bodies like the Moon record an earlier intense bombardment period in the solar system's history.
There are three main types of volcanoes classified based on their activity and structure:
1) Active volcanoes erupt regularly, dormant volcanoes have erupted in the past but are now quiet, and extinct volcanoes are unlikely to erupt again due to lack of lava supply.
2) Shield volcanoes have broad, gentle slopes built by fluid lava flows. Composite volcanoes have a steep, conical shape formed from layers of hardened lava and ash.
3) Examples include Mauna Loa, a shield volcano in Hawaii, and Mount St. Helens, a composite volcano in Washington, USA.
This document describes different types of intrusive volcanic rocks. It defines batholiths as large irregular reservoirs of magma that cool slowly underground. Laccoliths are dome-shaped intrusions that push up rock layers as magma is blocked below. Sills are horizontal sheets that form between bedding planes, while dikes are vertical or diagonal intrusions that cut across bedding planes. In conclusion, intrusive volcanism occurs when magma enters and solidifies in weaknesses or chambers in the earth's crust.
Volcanoes (GENEVEVE MAGPATOC & JORDAN ABRAHAM)magene
Volcanoes form at three main types of plate boundaries: divergent boundaries where plates split apart, convergent boundaries where one plate subducts beneath another, and at hotspots within plates. The type of boundary controls the composition of magma erupted - divergent boundaries produce basalt, convergent produce andesite, and hotspots can produce either depending on the plate composition. Major hazards from volcanoes include lava flows, explosive eruptions of ash and pyroclastic flows, lahars, and gas emissions. Large eruptions can impact global climate through atmospheric dust veiling sunlight. Volcanoes are monitored to determine activity levels and eruptions can be predicted based on increased seismicity, gas emissions,
There are 3 main types of volcanoes: composite volcanoes, cinder cones, and shield volcanoes. There are also 5 special case volcanoes: caldera volcanoes, mega-volcanoes, spatter cones, dome volcanoes, and lava plateaus. The document discusses the characteristics of each type of volcano.
Volcanology is the study of volcanoes, lava, magma, and related geological phenomena. A volcano forms when magma rises from deep in the Earth's mantle and erupts on the surface. As more magma rises, it forms a magma chamber and conduit leading to a vent. Eruptions through the vent build the volcano over time. There are four main types of volcanism related to mid-ocean ridges, subduction zones, hotspots, and flood volcanism. Heat sources for volcanism include radioactive decay, accretion during planetary formation, tidal effects, and core formation deep within the Earth.
The document describes different features of two main types of volcanoes: composite volcanoes and shield volcanoes. Composite volcanoes have thick, sticky lava and steep slopes, while experiencing very violent eruptions. Shield volcanoes contain thin, runny lava and have gentle slopes, forming from less violent eruptions. The document includes diagrams of the volcano types and tasks for students to label features and compare the characteristics of composite and shield volcanoes.
A volcano is a vent in the Earth's surface that allows magma, lava, gases, and pieces of rock to erupt out. Volcanoes occur near the boundaries of the Earth's tectonic plates as they push together or pull apart. They can be active and currently erupting, dormant if not erupting recently but capable of future eruptions, or extinct if no future eruptions are expected.
This document provides an overview of impact cratering mechanics and morphology. It explains that when objects impact planetary surfaces, they release enormous amounts of kinetic energy that excavates craters. There are two main types of craters - simple bowl-shaped craters and more complex craters with interior structures like terraces and central peaks. The size and morphology of craters depends on factors like the impacting object's energy, the planet's gravity, and the properties of the surface materials. Heavily cratered surfaces on bodies like the Moon record an earlier intense bombardment period in the solar system's history.
There are three main types of volcanoes classified based on their activity and structure:
1) Active volcanoes erupt regularly, dormant volcanoes have erupted in the past but are now quiet, and extinct volcanoes are unlikely to erupt again due to lack of lava supply.
2) Shield volcanoes have broad, gentle slopes built by fluid lava flows. Composite volcanoes have a steep, conical shape formed from layers of hardened lava and ash.
3) Examples include Mauna Loa, a shield volcano in Hawaii, and Mount St. Helens, a composite volcano in Washington, USA.
This document describes different types of intrusive volcanic rocks. It defines batholiths as large irregular reservoirs of magma that cool slowly underground. Laccoliths are dome-shaped intrusions that push up rock layers as magma is blocked below. Sills are horizontal sheets that form between bedding planes, while dikes are vertical or diagonal intrusions that cut across bedding planes. In conclusion, intrusive volcanism occurs when magma enters and solidifies in weaknesses or chambers in the earth's crust.
Volcanoes (GENEVEVE MAGPATOC & JORDAN ABRAHAM)magene
Volcanoes form at three main types of plate boundaries: divergent boundaries where plates split apart, convergent boundaries where one plate subducts beneath another, and at hotspots within plates. The type of boundary controls the composition of magma erupted - divergent boundaries produce basalt, convergent produce andesite, and hotspots can produce either depending on the plate composition. Major hazards from volcanoes include lava flows, explosive eruptions of ash and pyroclastic flows, lahars, and gas emissions. Large eruptions can impact global climate through atmospheric dust veiling sunlight. Volcanoes are monitored to determine activity levels and eruptions can be predicted based on increased seismicity, gas emissions,
There are 3 main types of volcanoes: composite volcanoes, cinder cones, and shield volcanoes. There are also 5 special case volcanoes: caldera volcanoes, mega-volcanoes, spatter cones, dome volcanoes, and lava plateaus. The document discusses the characteristics of each type of volcano.
Volcanology is the study of volcanoes, lava, magma, and related geological phenomena. A volcano forms when magma rises from deep in the Earth's mantle and erupts on the surface. As more magma rises, it forms a magma chamber and conduit leading to a vent. Eruptions through the vent build the volcano over time. There are four main types of volcanism related to mid-ocean ridges, subduction zones, hotspots, and flood volcanism. Heat sources for volcanism include radioactive decay, accretion during planetary formation, tidal effects, and core formation deep within the Earth.
The document describes different features of two main types of volcanoes: composite volcanoes and shield volcanoes. Composite volcanoes have thick, sticky lava and steep slopes, while experiencing very violent eruptions. Shield volcanoes contain thin, runny lava and have gentle slopes, forming from less violent eruptions. The document includes diagrams of the volcano types and tasks for students to label features and compare the characteristics of composite and shield volcanoes.
The document summarizes the four main types of rocks in the rock cycle: igneous, sedimentary, metamorphic, and their key characteristics. Igneous rocks form from cooling magma and have small or large crystals depending on cooling rate. Sedimentary rocks form through cementation of sediments and contain visible pieces of other materials. Metamorphic rocks were once igneous or sedimentary rocks that were buried deep underground and subjected to heat and pressure, changing their structure and forming intergrown crystals. The rock cycle shows how the different rock types are interrelated and can transform into one another over time through geological processes.
Volcanoes form at plate boundaries as molten rock, or magma, rises from below the Earth's crust. There are three main types of volcanoes: shield volcanoes which erupt fluid basalt and form wide gentle slopes, composite volcanoes which contain trapped gases and alternate between explosive and effusive eruptions forming steep slopes, and cinder cone volcanoes which have short eruptions of explosive ash and form small, steep cones. Volcanic eruptions produce hazards like pyroclastic flows, lahars, ash falls, and different types of lava. While eruptions can be locally devastating, volcanoes also create new land and leave nutrient-rich soils after erupting.
This document discusses different types of tectonic landscapes formed by extrusive igneous activity. It outlines lava plateaus like the Deccan Plateau and different types of volcanoes. The type of volcano depends on the lava composition, eruption type, and plate tectonic setting. Shield volcanoes are associated with basaltic eruptions at divergent boundaries. Composite and stratovolcanoes are associated with andesitic eruptions at convergent boundaries. Examples of different volcano types and their key features are provided.
Study guide in science 5 for third quarterCherrie Pie
1. The document discusses different types of rocks and how they are formed through various geological processes like weathering and the rock cycle. It also covers simple machines like levers, inclined planes, screws, and wheels and axles.
2. Key points include how tiny plants contribute to weathering of rocks through acid production, examples of weathering forces, and how soil supports plant growth. Simple machines make work easier, faster and better by reducing the amount of force needed.
3. Different types of rocks like igneous, sedimentary and metamorphic rocks form through melting, compaction of sediments, and changes induced by heat and pressure.
Volcanoes are openings in the earth's crust that eject lava, pyroclasts, and gases during eruptions. There are three main types of volcanoes: shield volcanoes, cinder cone volcanoes, and composite or stratovolcanoes. Cinder cone volcanoes are small, steep-sided hills made of loose cinders ejected during eruptions. Volcanic eruptions can be either explosive or violent, ejecting pyroclasts and ash, or quiet and non-explosive, with gentle lava flows.
The rock cycle document describes the three main types of rocks - igneous, sedimentary, and metamorphic - and how they are related through geological processes. It focuses on igneous rocks, which form from cooling magma, and can cool underground to form intrusive rocks or above ground to form extrusive rocks like lava. The composition and cooling rate of magma determines the type of igneous rock formed. Magma is hot melted rock from deep in the Earth, and its viscosity is affected by temperature and silica content.
There are three main types of volcanoes that form from different geological processes:
1) Hotspot volcanoes like those in Hawaii form when magma rises from a hotspot in the mantle as a tectonic plate moves over it. Eruptions are less explosive due to fluid magma.
2) Shield volcanoes form at divergent plate boundaries and from hotspots, with low, wide shapes from fluid basaltic magma.
3) Composite volcanoes form at convergent plate boundaries, where one plate subducts under another. They have steep sides due to more viscous magma and explosive eruptions, producing hazards like pyroclastic flows and lahars.
1) Alfred Wegener proposed the continental drift theory which stated that the Earth was once a single supercontinent called Pangaea surrounded by an ocean.
2) Evidence for continental drift includes fossils of the same plants and animals found on different continents, matching rock formations, and glacial deposits found in areas that were once near the South Pole.
3) Arthur Holmes suggested thermal convection in the Earth's mantle as the driving force behind continental movement, likening it to a conveyor belt. This led to the development of the theory of plate tectonics.
293 11 30_20078th grade science study guide 1alfskill
The document provides information about various topics in 8th grade science including earth and space science, physical science, and earth science. It covers concepts such as the rotation and revolution of Earth, seasons, eclipses, gravity, tools used to study space, the rock cycle, plate tectonics, forces and motion. Key ideas are presented through definitions, diagrams, and examples. Sample questions are also included to help with studying.
This presentation discusses volcanoes and was created by students from Holy Family Balika Vidyalaya in Wennappuwa, Sri Lanka. It defines a volcano, explains why they are created through tectonic plate movement, describes the interior of volcanoes and how magma travels through them. It provides a world map of volcanoes and defines several types of volcanoes. A table lists some of the most continuously active volcanoes and their locations. The presentation discusses both negative effects like ash falls and landslides as well as positive effects like nutrient deposits. It concludes with highlighting the devastating eruption of Mount Vesuvius that buried the cities of Pompeii and Herculaneum in 79 AD.
This document discusses different types of volcanoes. It provides descriptions of cinder cones, shield volcanoes, composite volcanoes, and lava domes. Cinder cones are symmetrical cones up to 1,200 feet tall formed from a single vent. Shield volcanoes are very broad with shallow slopes and can be over 30,000 feet tall. Composite volcanoes are also known as stratovolcanoes, ranging from 1-10 km wide and up to 10,000 feet tall with steep slopes. They have explosive, dangerous eruptions. Lava domes are much smaller formations that occur when lava is too viscous to flow, piling up in a dome shape around 100 feet tall. Examples of each type
Volcanoes are formed when molten rock, or magma, rises up from below the Earth's surface through cracks, called vents, caused by the movement of tectonic plates. The magma exits through these vents and creates landforms on the surface, such as craters at the top of volcanoes. Volcanoes can be classified as active if they erupt frequently, extinct if they were once active but will not erupt again, or dormant if they were previously active but have not erupted recently, although future eruptions are possible.
This document provides information about a station-based volcano education program. The stations cover topics like classifying volcanoes, eruption types, magma composition, and volcanic hazards and benefits. At each station, students fill out worksheets or do activities to learn about parts of volcanoes, what causes eruptions, how silica and water content determine explosivity, different lava and pyroclastic material types, and examples of shield, cinder cone, and composite volcanoes. Math problems calculate totals, differences, distances, times, costs, and rates related to volcanic eruptions, ash and lava flows, and operating robots. The goal is to help students understand volcanoes through hands-on activities at multiple informative stations.
Is there a 9th planet heading for Earth?Ed Excluss
Much talk about planet 9 (Nibiru) But is it true? Well something is affecting our solar system, for sure. Here are the facts and myths in simple terms about planet X, Nibiru or whatever you call it
Volcanoes form when magma rises up from the Earth's mantle and crust and erupts. There are three main types of volcanoes defined by their activity level - active volcanoes that are currently erupting or may erupt soon, dormant volcanoes that have not erupted in a long time, and extinct volcanoes that have not erupted for over 10,000 years. Volcanic eruptions expel gases, ash, lava, and other materials from the vent of the volcano. The movement of tectonic plates is responsible for volcanism in many parts of the world.
Volcanoes occur primarily at plate boundaries and above hot spots in the mantle. There are currently around 1,500 active volcanoes worldwide. Volcanoes can be classified based on their structure and eruption type as shield volcanoes, cinder cone volcanoes, or composite volcanoes. The style of a volcanic eruption depends on factors like the amount of water vapor, trapped gases, and magma composition.
This document defines volcanoes as openings in the Earth's crust that allow molten rock and gases to escape. It notes that over half of the world's active volcanoes above sea level are located along the Ring of Fire. Volcanoes form when tectonic plates collide, spread apart, or interact under a plate. The parts of a volcano include the crater, pipe, cone, and vent. There are three main types of volcanoes: composite/strato volcanoes, shield volcanoes, and cinder cone volcanoes. Volcanic eruptions can have both beneficial effects like adding nutrients to soil or creating new islands, and harmful effects like releasing aerosols or abandoning land.
This document proposes a 3D printed Martian habitat called Outpost Olympus that would be constructed primarily using materials found on Mars. It describes a structural frame that would be printed from continuous basalt composite rods produced by melting and drawing Martian basalt fibers. The frame would form the foundation for environmental protection layers like parachute fabric, sealant, and regolith shielding. The habitat would be designed for long-term livability with separate crew quarters, laboratories, and life support systems to support 4 inhabitants for at least 1 year.
The document discusses plans for building a human civilization on Mars. It describes how materials available on Mars like soil, sulfur and carbon dioxide can be used to produce concrete, oxygen, and electricity. Concrete can be made from Martian soil and molten sulfur without needing water. A device called MOXIE will produce oxygen from the carbon dioxide-rich atmosphere. Electricity could come from the planetary core through graphene conductors in a project called Limitless Energy. Food would need to be grown on Mars through sustainable agriculture once colonies are established. The document outlines necessary innovations and resources to build shelters, life support systems, and a self-sufficient infrastructure for human settlements on Mars.
Lunar Habitation PPTX (Anyone can use it without permission)varunrajavr1
Lunar habitation refers to building human habitable structures on the moon. Constructing a lunar habitat requires gathering construction materials from the lunar surface like lunar regolith. Robots can be used as workers to build habitats from these materials more efficiently than human laborers in space suits. The habitats could be built underground in lava tubes for temperature control and protection. Operating a lunar habitat requires managing food production, extracting and purifying water, generating oxygen, removing carbon dioxide, monitoring air quality, and properly disposing of waste.
The document summarizes the four main types of rocks in the rock cycle: igneous, sedimentary, metamorphic, and their key characteristics. Igneous rocks form from cooling magma and have small or large crystals depending on cooling rate. Sedimentary rocks form through cementation of sediments and contain visible pieces of other materials. Metamorphic rocks were once igneous or sedimentary rocks that were buried deep underground and subjected to heat and pressure, changing their structure and forming intergrown crystals. The rock cycle shows how the different rock types are interrelated and can transform into one another over time through geological processes.
Volcanoes form at plate boundaries as molten rock, or magma, rises from below the Earth's crust. There are three main types of volcanoes: shield volcanoes which erupt fluid basalt and form wide gentle slopes, composite volcanoes which contain trapped gases and alternate between explosive and effusive eruptions forming steep slopes, and cinder cone volcanoes which have short eruptions of explosive ash and form small, steep cones. Volcanic eruptions produce hazards like pyroclastic flows, lahars, ash falls, and different types of lava. While eruptions can be locally devastating, volcanoes also create new land and leave nutrient-rich soils after erupting.
This document discusses different types of tectonic landscapes formed by extrusive igneous activity. It outlines lava plateaus like the Deccan Plateau and different types of volcanoes. The type of volcano depends on the lava composition, eruption type, and plate tectonic setting. Shield volcanoes are associated with basaltic eruptions at divergent boundaries. Composite and stratovolcanoes are associated with andesitic eruptions at convergent boundaries. Examples of different volcano types and their key features are provided.
Study guide in science 5 for third quarterCherrie Pie
1. The document discusses different types of rocks and how they are formed through various geological processes like weathering and the rock cycle. It also covers simple machines like levers, inclined planes, screws, and wheels and axles.
2. Key points include how tiny plants contribute to weathering of rocks through acid production, examples of weathering forces, and how soil supports plant growth. Simple machines make work easier, faster and better by reducing the amount of force needed.
3. Different types of rocks like igneous, sedimentary and metamorphic rocks form through melting, compaction of sediments, and changes induced by heat and pressure.
Volcanoes are openings in the earth's crust that eject lava, pyroclasts, and gases during eruptions. There are three main types of volcanoes: shield volcanoes, cinder cone volcanoes, and composite or stratovolcanoes. Cinder cone volcanoes are small, steep-sided hills made of loose cinders ejected during eruptions. Volcanic eruptions can be either explosive or violent, ejecting pyroclasts and ash, or quiet and non-explosive, with gentle lava flows.
The rock cycle document describes the three main types of rocks - igneous, sedimentary, and metamorphic - and how they are related through geological processes. It focuses on igneous rocks, which form from cooling magma, and can cool underground to form intrusive rocks or above ground to form extrusive rocks like lava. The composition and cooling rate of magma determines the type of igneous rock formed. Magma is hot melted rock from deep in the Earth, and its viscosity is affected by temperature and silica content.
There are three main types of volcanoes that form from different geological processes:
1) Hotspot volcanoes like those in Hawaii form when magma rises from a hotspot in the mantle as a tectonic plate moves over it. Eruptions are less explosive due to fluid magma.
2) Shield volcanoes form at divergent plate boundaries and from hotspots, with low, wide shapes from fluid basaltic magma.
3) Composite volcanoes form at convergent plate boundaries, where one plate subducts under another. They have steep sides due to more viscous magma and explosive eruptions, producing hazards like pyroclastic flows and lahars.
1) Alfred Wegener proposed the continental drift theory which stated that the Earth was once a single supercontinent called Pangaea surrounded by an ocean.
2) Evidence for continental drift includes fossils of the same plants and animals found on different continents, matching rock formations, and glacial deposits found in areas that were once near the South Pole.
3) Arthur Holmes suggested thermal convection in the Earth's mantle as the driving force behind continental movement, likening it to a conveyor belt. This led to the development of the theory of plate tectonics.
293 11 30_20078th grade science study guide 1alfskill
The document provides information about various topics in 8th grade science including earth and space science, physical science, and earth science. It covers concepts such as the rotation and revolution of Earth, seasons, eclipses, gravity, tools used to study space, the rock cycle, plate tectonics, forces and motion. Key ideas are presented through definitions, diagrams, and examples. Sample questions are also included to help with studying.
This presentation discusses volcanoes and was created by students from Holy Family Balika Vidyalaya in Wennappuwa, Sri Lanka. It defines a volcano, explains why they are created through tectonic plate movement, describes the interior of volcanoes and how magma travels through them. It provides a world map of volcanoes and defines several types of volcanoes. A table lists some of the most continuously active volcanoes and their locations. The presentation discusses both negative effects like ash falls and landslides as well as positive effects like nutrient deposits. It concludes with highlighting the devastating eruption of Mount Vesuvius that buried the cities of Pompeii and Herculaneum in 79 AD.
This document discusses different types of volcanoes. It provides descriptions of cinder cones, shield volcanoes, composite volcanoes, and lava domes. Cinder cones are symmetrical cones up to 1,200 feet tall formed from a single vent. Shield volcanoes are very broad with shallow slopes and can be over 30,000 feet tall. Composite volcanoes are also known as stratovolcanoes, ranging from 1-10 km wide and up to 10,000 feet tall with steep slopes. They have explosive, dangerous eruptions. Lava domes are much smaller formations that occur when lava is too viscous to flow, piling up in a dome shape around 100 feet tall. Examples of each type
Volcanoes are formed when molten rock, or magma, rises up from below the Earth's surface through cracks, called vents, caused by the movement of tectonic plates. The magma exits through these vents and creates landforms on the surface, such as craters at the top of volcanoes. Volcanoes can be classified as active if they erupt frequently, extinct if they were once active but will not erupt again, or dormant if they were previously active but have not erupted recently, although future eruptions are possible.
This document provides information about a station-based volcano education program. The stations cover topics like classifying volcanoes, eruption types, magma composition, and volcanic hazards and benefits. At each station, students fill out worksheets or do activities to learn about parts of volcanoes, what causes eruptions, how silica and water content determine explosivity, different lava and pyroclastic material types, and examples of shield, cinder cone, and composite volcanoes. Math problems calculate totals, differences, distances, times, costs, and rates related to volcanic eruptions, ash and lava flows, and operating robots. The goal is to help students understand volcanoes through hands-on activities at multiple informative stations.
Is there a 9th planet heading for Earth?Ed Excluss
Much talk about planet 9 (Nibiru) But is it true? Well something is affecting our solar system, for sure. Here are the facts and myths in simple terms about planet X, Nibiru or whatever you call it
Volcanoes form when magma rises up from the Earth's mantle and crust and erupts. There are three main types of volcanoes defined by their activity level - active volcanoes that are currently erupting or may erupt soon, dormant volcanoes that have not erupted in a long time, and extinct volcanoes that have not erupted for over 10,000 years. Volcanic eruptions expel gases, ash, lava, and other materials from the vent of the volcano. The movement of tectonic plates is responsible for volcanism in many parts of the world.
Volcanoes occur primarily at plate boundaries and above hot spots in the mantle. There are currently around 1,500 active volcanoes worldwide. Volcanoes can be classified based on their structure and eruption type as shield volcanoes, cinder cone volcanoes, or composite volcanoes. The style of a volcanic eruption depends on factors like the amount of water vapor, trapped gases, and magma composition.
This document defines volcanoes as openings in the Earth's crust that allow molten rock and gases to escape. It notes that over half of the world's active volcanoes above sea level are located along the Ring of Fire. Volcanoes form when tectonic plates collide, spread apart, or interact under a plate. The parts of a volcano include the crater, pipe, cone, and vent. There are three main types of volcanoes: composite/strato volcanoes, shield volcanoes, and cinder cone volcanoes. Volcanic eruptions can have both beneficial effects like adding nutrients to soil or creating new islands, and harmful effects like releasing aerosols or abandoning land.
This document proposes a 3D printed Martian habitat called Outpost Olympus that would be constructed primarily using materials found on Mars. It describes a structural frame that would be printed from continuous basalt composite rods produced by melting and drawing Martian basalt fibers. The frame would form the foundation for environmental protection layers like parachute fabric, sealant, and regolith shielding. The habitat would be designed for long-term livability with separate crew quarters, laboratories, and life support systems to support 4 inhabitants for at least 1 year.
The document discusses plans for building a human civilization on Mars. It describes how materials available on Mars like soil, sulfur and carbon dioxide can be used to produce concrete, oxygen, and electricity. Concrete can be made from Martian soil and molten sulfur without needing water. A device called MOXIE will produce oxygen from the carbon dioxide-rich atmosphere. Electricity could come from the planetary core through graphene conductors in a project called Limitless Energy. Food would need to be grown on Mars through sustainable agriculture once colonies are established. The document outlines necessary innovations and resources to build shelters, life support systems, and a self-sufficient infrastructure for human settlements on Mars.
Lunar Habitation PPTX (Anyone can use it without permission)varunrajavr1
Lunar habitation refers to building human habitable structures on the moon. Constructing a lunar habitat requires gathering construction materials from the lunar surface like lunar regolith. Robots can be used as workers to build habitats from these materials more efficiently than human laborers in space suits. The habitats could be built underground in lava tubes for temperature control and protection. Operating a lunar habitat requires managing food production, extracting and purifying water, generating oxygen, removing carbon dioxide, monitoring air quality, and properly disposing of waste.
1. The document provides background information on impact craters, describing their typical structure and how they are formed by asteroid and comet impacts. It explains that larger craters have more complex structures like central peaks or terraces.
2. An activity is described where students will create impact craters by dropping objects into boxes containing layered materials like sand and paint. This allows them to observe how the size and speed of the impactor affects the resulting crater and ejecta pattern.
3. Key parts of impact craters are defined, and different types of craters from simple to complex and multi-ring basins are described. Examples of famous impact craters on Earth and the Moon are also given.
2- When we think about cratering- we usually think of big rocks fallin.docxStephenSR9Ramplingv
2. When we think about cratering, we usually think of big rocks falling onto a planet, but even tiny pebbles can make craters. Near the footprint in the above picture, you can see many small "pock-marks." These marks are the craters made by microscopic particles that hit the surface moving at speeds of several kilometers per second. Marks like these cannot be found on the Earth's surface. Why not? List two different reasons. 3. Craters accumulate over time. This means that the number of craters you see gives a rough idea of the age of the surface. Using this method, sort the surfaces of Venus, Earth, Mercury, Mars and the Moon by age from oldest surface via crater counting to youngest. 4. How can you reconcile these vastly different ages of surfaces with the idea that all the planets formed at the same time? Part 2: Volcanism Around the Solar System Volcanism can be very important in shaping the surface features of a planet. Venus has a large number of unique volcanic features. On Earth, when volcanoes erupt, the molten lava within them can travel great distances before it cools. However, on Venus, molten lava does not travel very far before it cools. Compare these examples of shield volcanoes on Venus and on Earth. 5. Volcanoes on Venus and Earth look different. Compare and contrast the pancake volcanoes with the shield. Give at least two examples. 6. What might cause those differences between the two planets?
.
Oceanography 100 Reading and Homework Assignments – Chapter 1(Se.docxhopeaustin33688
Oceanography 100 Reading and Homework Assignments – Chapter 1
(See schedule for due dates)
Chapter 1:Read the entire chapter. Also read Appendix III.
Vocabulary (for studying purposes only):
Ocean
Sea
Sextant
Latitude
Longitude
http://blog.worldlabel.com/2009/clip-art-of-the-week-papapishus-junk-ship-and-wikimedia-clips.html
Sir James Cook
The Scientific Method
Hypothesis vs. Theory
Nebular Hypothesis
Density
Density Stratification
Earth’s Chemical Layers
Crust (oceanic vs. continental)
Mantle
Outer Core
Inner Core
Earth’s Physical Layers
Lithosphere
http://www.teachengineering.org/view_activity.php?url=http://www.teachengineering.org/collection/cub_/activities/cub_navigation/cub_navigation_lesson10_activity1.xml
Asthenosphere
Lower Mantle
Isostatic Adjustment
Isostatic Rebound
Outgassing
Stanley Miller
Atmosphere
Photosynthesis vs. Respiration
Oxidation Event
Radiometric Dating
Half-life
Geologic Time Scale
Homework:
1) (Concept Check 1.2, #3) List some of the major achievements of Captain James Cook.
2) T or F? The deepest place in the ocean, the Marianas Trench, is not as deep as the highest place on land is tall. In other words, if we put Mt. Everest in the Marianas Trench the top would stick out above water to form an island.
3) On the diagram below, color/highlight the lines of latitude with red or pink, the lines of longitude with blue. Then, answer the following questions with either latitude, longitude, or both. Note, the handout and Appendix III are the place to look for these answers.
N
a) Form circles around the Earth. __________________
b) 0° is located at the Equator __________________
c) 1° can be divided into 60’ or 3600’’__________________
d) Measured in ° east or west of the prime meridian.
__________________
4) Which of the following locations is farthest north? A) Newest Town 35° 45” N, 45° 35’ W b) Oldest Town 15° 55’ S, 15° 5’ W c) Youngstown 25° 58” N, 5° 35’ E
5) T or F? Our solar system formed about 45 Billion years ago.
6) Outline the steps believed to occur in the formation of a solar system by the Nebular Hypothesis (also called the solar nebula hypothesis). What is nuclear fusion and how does it relate to the Nebular Hypothesis?
7) Density stratification refers to the formation of layers due to differences in density. Complete the chart of the Earth’s chemical layers and their composition (below).
Layer Name
Sub layer
Composition
Depth to Top
Depth to Bottom
Crust
Oceanic
Continental
Mantle
Core
Outer Core
Inner Core
8) Geoscientists also divide the Earth into layers based on differences in the way these layers behave (physical properties). Fill in the blanks below using the terms asthenosphere. lithosphere, or lower mantle (mesosphere).
a. Top layer _________________
b. Oozy layer _________________
c. Layer below the asthenosphere _________________
d. Rigid / brittle layer _________________
.
This document discusses colonization of Mars and terraforming the planet. It outlines the need for colonization, including population growth and making humans a multiplanetary species. Mars is a potential target for colonization due to its proximity and similarities to Earth. However, living on Mars presents challenges like low temperatures, thin atmosphere, and high radiation. The document proposes methods for terraforming Mars, including using orbital mirrors to increase sunlight and warming, importing ammonia-rich asteroids to add greenhouse gases, and producing halocarbon gases. Each method aims to make Mars' environment more hospitable for human life.
A Space Suit for Extra Ordinary Martian Conditions 1Can Kural
A space suit designed specifically for exploring Mars is proposed that addresses the challenges of the Martian environment. The suit would have multiple protective layers, including an inner gravity skin suit to mitigate muscle and bone loss. The outer layers would protect against dust storms and radiation. Systems would be embedded in the suit layers to recycle waste and provide life support through a tight-fitting biometric counter-pressure suit and helmet. The suit would be designed for flexibility and reliability through localized self-repair capabilities while maintaining overall system integrity.
Here are the responses to complete the sentences:
4. When an oceanic plate collides with a continental plate WORD LIST
the oceanic plate goes under the continental plate. rocks
This happens because the oceanic is heavier. extinct
5. As it goes under, the higher temperature of the mantle melts it volcano
and the magma rises up through cracks as dikes. This is lava
how a subduction zone is formed. oceanic
steam
6. Five things that pour out of a volcano during an eruption are active
lava, ash, steam, dust dust
and magma. continental
dormant
7. An active volcano is
The document provides information on the formation and anatomy of the Earth. It begins with a summary of the Big Bang theory and steady state theory of the origin of the universe. It then discusses the formation of the early Earth through accretion and differentiation of layers. It provides details on the structure of the Earth, including the lithosphere, mantle, outer core, and inner core. It also discusses plate tectonics, including plate boundaries, faulting, folding, volcanoes, and earthquakes. Additional topics covered include the water cycle, denudation processes, and natural landscapes.
The interstellar medium is the matter that exists between stars in galaxies, consisting of gas and microscopic dust particles. About 1% of a galaxy's mass is made up of interstellar medium. In the Milky Way, the density of the interstellar medium is about 1 atom per cubic centimeter, much less dense than Earth's atmosphere. Molecular clouds within the interstellar medium can be enormous, many light years across and containing thousands of times the mass of the Sun. The interstellar medium plays an important role in the formation of stars, planets and other astronomical objects.
This document summarizes research on the habitable zones around stars and the habitability of exoplanets. It discusses how the habitable zone is defined as the region where liquid water could exist on a planet's surface. The inner and outer edges of the habitable zone are modeled based on factors like the runaway greenhouse effect and CO2 condensation limits. Current exoplanet detection methods are also overviewed. While over 20 potentially habitable exoplanets have been identified, confirming life remains difficult due to natural phenomena creating false biosignatures. However, an inhabited exoplanet may be confirmed in the near future as detection capabilities continue advancing rapidly.
The document proposes a student research project called "Swachch Antariksh" to collect magnetic space debris using an electromagnet onboard a satellite. The satellite would orbit Earth collecting small debris in an aluminum alloy net and periodically depositing it. Collected debris could be disposed of in a graveyard orbit or the South Pacific Ocean. The project aims to reduce risks posed by the growing amount of orbital debris and enable continued space exploration.
The formation of the solar system began from a large cloud of gas and dust called the solar nebula. As the nebula collapsed due to gravity, it formed a disc with the sun at the center. Planetesimals within the disc collided and accreted to form the planets. The nebular theory explained many characteristics of the solar system but did not account for all observations. The modern condensation theory expanded on this model and better explained features such as the asteroid belt and comets through processes like condensation and fractionation within the early solar system.
Mars One is planning a one-way mission in 2024 to colonize Mars with crews of four departing every two years. While Mars has similarities to Earth like polar ice caps and length of day, it poses challenges for human habitation including extreme cold, low atmospheric pressure, dust storms, and lack of liquid water. Long term, colonizing Mars could help ensure humanity's survival if Earth becomes uninhabitable when the expanding sun boils away our oceans in billions of years. However, establishing permanent settlements on Mars presents numerous technological and biological hurdles that must be overcome.
Astronomy notes2: Notes on the composition & formation of Galaxies, leading ...Robin Seamon
1) The document is a set of astronomy lecture notes that covers topics including the universe, galaxies, stars, planets, and Earth's formation.
2) It begins by discussing how the universe began with the Big Bang and covers vast distances in space measured in light years.
3) Key details are provided about the solar system and its planets, along with facts about each planet's characteristics such as length of day/year, temperature, and composition. Diagrams and links are included for reference.
We can arrive at this strategy after observing the historic lunar missions and the
data available in the public domain. This document shall present the thought process,
logical and mathematical derivations by which Chandrabhraman has arrived to following
mentioned Landing Sites. It shall conclude with the results that would show various
proposed Landing sites.
This document discusses light years and how they are used to measure distance. A light year is defined as the distance that light travels in one year, which is approximately 5,865,696,000,000 miles. The document then provides background on the Big Bang theory, explaining that it describes how the universe began in a hot, dense state and has been expanding ever since. It lists several pieces of evidence that support the Big Bang model, such as the cosmic microwave background radiation and abundance of light elements like hydrogen and helium.
This document provides instructions for a lab on isostasy and plate tectonics. It introduces concepts like isostatic equilibrium, where crust "floats" on the mantle based on relative densities, and how this explains Earth's bimodal topography. It then discusses plate tectonics, noting that earthquakes define plate boundaries and volcanism occurs at boundaries. Finally, it covers the three types of plate boundaries - divergent at mid-ocean ridges, convergent at destructive margins, and transform - and how to calculate plate velocities using hotspot and seafloor age data.
space suits their materials and fabrication technique and space age suiting.
Embark on a journey through the cosmos as we delve into the cutting-edge realm of space suit textiles. Our presentation is a captivating exploration of the evolution, advancements, and future possibilities of the fabrics that shield astronauts in the unforgiving vacuum of space.
Discover the technological marvels that make modern space suits a blend of comfort, functionality, and life-saving capabilities. From the early days of space exploration to the latest breakthroughs, our presentation offers a comprehensive overview of the materials and design principles that have shaped the iconic suits worn by astronauts.
Immerse yourself in the fascinating world of multi-layered fabrics engineered to withstand extreme temperatures, radiation, and microgravity. Learn about the intricate balance between flexibility and durability that these textiles achieve, ensuring astronauts can maneuver with precision while staying protected in the harsh conditions of space.
Explore the integration of smart textiles and sensors, providing real-time data on an astronaut's vital signs and environmental conditions. Witness how these technological enhancements contribute to the overall safety and success of space missions.
1. Episode #1: Bubba and Robbi go to Mars
“Robby” the Robot “Astro” the astronaut “Bubba” the bubbleThe voice of reason The planning team
Scalable construction
Dynamic multi-purpose space -> increased standard of living
Exploit local climate to our benefit
Mars conditions
are harsh. From
low atmospheric
pressure to cold
temperatures.
We need to
optimize for
success.
Well, when you put it like that.
I guess I could get rid of my
pool table and pinball machine.
1
Energy efficient morphology
100 m3
100 m3
3X surface
X surface
Function over formBring small amounts of high performance
materials/ technologies from earth
Selective use of 3D printing -> effectivity
No, Robby, we
are only printing
critical parts of
the home. We
aren’t printing
things just for
the sake of
printing them...
If you don’t have a gym
on Mars, you will get
muscle atrophy and die.
Time advantage. Time is cheap
Relax! It will take
you at least a year
to commute there.Plus
another
decade to
build the
technology
It is going to take
you HOW MANY
YEARS to build my
home on Mars?!
High redundancy in the construction process - aka survivability!
THE 3DP ADVENTURES OF
CORE
CONCEPTS
starring
TECH
ARCH
Can I 3D
print a skull?
Please,
please,
please!!! All
of the new
3D printers
are printing
them!
Social dynamics -> Varying degrees of public and private spaces
private
public
I think
BFF’s joined
at the hip
we’re cool
we’ve met
before
Anything from
composite to digital
materials to 3D printed
bio-mimicri structures.
My only
shovel
broke
We don’t want this to
happen to us on Mars.
That is why there is a
plan C in case plans A
and B fail.
2. Valles Marineris
Bubba
Predesigned structural voids are filled
with Martian soil for constructive support
I found it! The
perfect place :)
Thicker atmosphere,
water potential and
lots to research!
Come on guys, umm...
I mean rovers! Fill
this bubble up with
Martian sand.
After I’m filled with sand, I’m
covered with another layer of
sand and a brick dome, for
protection against meteors
and radiation. Now sintering
brick #23B
I go around Mars looking for
quartz rich sand I can
sinter. Then I sinter it into
a brick and carry it to its
corresponding location within
the brick dome.
We chose
semi-
buried.
But it
could also
be...
Has anyone seen
a good crater
around here?!
Bubble
Concept overview
Self transporting habitat
The exact bubble
will depend on
the micro-location.
Above ground (F*** radiation) Wedged in the side of a cliff
10 feet meters under, literally!
I have additional “side wings” that
can be inflated in stages based on
the width of the crater I find...
More
about
Bubba’s
location
later...
Find
crater
Inflate core
structure
Fill pillars and
base with sand
Inflate expand-
able wings
Cover with sand
and brick dome
See my top
view? My pillars
are filled with
sintered sand.
Lets keep driving
towards the optimal
crater the guys from
NASA found...
2
1
There are
. multiple
sinterning robots who
work in syncronization
to build the dome. This
also provides redun-
dancy in case one is
compromised.
A small gas container is released inside of
the bubble to expand it
2
3
4
5
We can bring very small
. amounts of gas due to the
extremely low atmospheric pressure
and Mars. This, together with low
gravity, facilitates easy inflation and
high relative internal pressure.
Like a caterpillar turning into a
butterfly, Bubba roams Mars in
compact rover form, expanding to full
capacity only once it finds a suitable location.
The essential technological systems are
combined inside the rover, and when inflated
become an active part of the habitat.
3. BUBBLE TECHNOLOGY
3
An Inflatable structure
Sinergy with additive sintering
Sophisticated Internal structure
Construction order / methodology
Mars atmospheric conditions are ideal for inflatable structures. The atmospheric pressure
. on ground level is 200X smaller then that on earth. This means that inflating a structure to
a certain pressure requires much less gas. Combining that with the gravity being one third of that on
earth, it is expected to take down the amount of gas needed by 600X to withstand the equivalent
mass on top of the structure compared to earth. This means that very little amounts of gas need to
be taken from earth for the inflation process if pumping is too energy intensive.
By predesigning the cut of the bubble, it is possible to fully control its spacial structure to any
desired shape, much beyond the standard bubble shape.
Inflating may be achieved by releasing gas containers prepositioned inside the bubble, that maintain
a constant pressure by use of smart passive valves made of digital materials that are pressure sensitive.
The bubble technology introduces a smart combination between in situ
. fabricationon Mars, and prefabrication on Earth.
Prefabrication utilizes most advanced technologies available on Earth. The sheet material
that makes the structure’s skin can be highly robust but light (i.e. composite fabrics),
introduces optimal behaviour for Martian conditions, and integrates energy supplying
systems within itself. It can have the optimal complexity and reliability to weight ratio.
In situ fabrication is used to create large mass parts of the construction that are nearly
impossible to bring from earth. They act mainly as an engineering skeleton of the
habitat, and critical mass for radiation blockage. Through this combination, we believe,
the most efficient and practical process can be achieved.
The inflated bubble conceptually acts as a supporting structure for an additive manufacturing
. process. This is done in two different manners. First, the constructional in situ voids act as guides
to the formation of pillars that hold the structure from collapsing under compressive stress. Second, the
entire inflated structure acts as a support to the formation of a dome structure that covers the entire
bubble. The air pressure inside the bubble, combined with the “in situ” pillars, introduce enough strength
to hold big amounts of sintered Martian sand, and even the weight of a rover climbing on top of it.
The complex structure of the bubble is naturally followed by a suitable construction methodology. As
described in previous pages, once positioned inside a crater the bubble is inflated, when successive layers
are selectively inflated to fill the existing gap between the bubble core and the crater’s surface. Further
gaps are covered with sand by the rovers to give them access to the top of the bubble from where they
can fill it with sand. Once fully inflated, the constructional in situ voids are filled with sand, and then the
more internal voids surrounded by the sand are filled with sintered/melted sand. The sand filling is done
by rovers by means of an articulated arm, a parallel cable robot, or by climbing on the bubble.
When the creation of in situ pillars is done, the formation of the sintered dome starts. The dome covers
the entire overground exposed area of the bubble and acts as protection from radiation, sand storms,
meteorites, and other elements.
Constructional In Situ Voids which are
. filled with Martian sand, either in a grain
form or sintered. Those voids are morphologically
external to the inflatable structure and have
direct contact with Mars’ atmosphere. Any void to
be filled with sintered sand is surrounded by non
sintered sand void, to avoid the hot sintered sand
from melting the bubble’s skin.
Habitat Voids, once populated, are then filled with
breathable air. Those make the biggest portion of
the habitat by volume.
Additional types of voids may be filled with
specialty materials, i.e. to supply further protec-
tion from radiation.
The inflated structure is constructed
. from several conceptual void types;
Together, the different void types make the
entire construction volume.
Constructional Gas Voids, in which the inflating
gas is released. When inflated, those voids act as
the constructional skeleton of the structure.
Insulation Gas Voids - Those act as a tempera-
ture insulation layer, they may be alternatively
absent of any gas (vacuumed) for optimal insula-
tion. Morphologically, they separate between the
habitat void and the Martian atmosphere and
Martian ground.
Prefabrication combined with in situ
4. What if we let
the bubbles fill
passively with
sand, because
of the dust
storms?
Love it! But that
might not be fast
enough... How about
that combined with
solar powered micro
pumps to fill the
bubbles...
Take that
Martian sand
storms!
Imagine a bubble that is passively filled with sand during Martian dust storms.
Dozens of these bubbles can be sent to Mars and thrown onto its surface. Over the years
they will passively stabilize themselves and become ready for habitation...
5. 1:75
We have a great idea for
creating a Mars habitat, but
where should we put it?!
Haughton crater on Devon
Island in Canada
You know what they
say about real estate,
LOCATION-LOCATION
-LOCATION!
We need a
practice site on
Earth, ASAP!
It has water aquifers and is a
great place to research. Plus
it isn’t as freezing or as hot
as the rest of Mars, since it is
near the equator.
On Mars we can settle in Valles Marineris.
Gobi desert in AsiaMcMurdo Dry
Valleys in Antarc-
tica
3D PRINTING
LOCATION
6
Low humidity, no snow
and 32o kph winds
Rapid temperature changes, up to
35 °C within 24 hours. -40°C in the
winter, +50°C in the summer
3D printing technology is primarily used to create large mass structures. In order to exploit the existing resources on Mars, sintering
technology is used. This technology combines the use of Martian soil that is sinterable, with available solar radiation that can be
optically condensed to produce sintering heat. Additionally, solar power converted to electricity may be used to control an XYZ manipu-
lator.
The 3d printing process is designed to have high redundancy. Several rovers may be used to mine the sinterable soil of Mars. Geared
with spectroscopy sensors, the rovers travel around the construction site looking for sinterable ground. When found, a predefined shape
of a “brick” is sintered by the rover on the spot. The brick is then transported by the rover to the construction site where it is
sintered to the back to the entire structure. When sintering the brick, existing rocks in the area may be used as volume fillers to
accelerate the production process. Therefore, the rover is geared with 3d scanning technology and algorithms to assess and understand
the geometry of a rock.
The rovers act as a group of mini-builders that communicate between themselves and a headquarters. They produce the bricks accord-
ing to a predefined plan in the right order to create a dome shape that will cover the bubble. The result is a manufacturing process
that can be dynamically distributed. It demonstrates high redundancy as it uses several similar mini-builders, and very flexible as each
body is created from smaller bricks.
The concept of 3D printed pillars inside an inflatable structure was further developed to demonstrate the creation of internal details
of the habitat. The core concept of sintered skeleton holding an inflatable structure can be used to create furniture such as tables
and chairs, or as local constructional support within the habitat. One can imagine that prior to landing on Mars, the 3D printing rovers
can manufacture sintered rods that will serve as raw material for the manual construction of more complex shapes.
The bubble concept allows us to exploit the revolution of 3D printing not only on Mars itself, but also
on Earth, as 3D printing may be used to easily manufacture complex inflatable structures such as the
proposed bubble.
Our first priority in choosing a location is to protect against exposure to the elements such as: climate profile, temperature
. extremes, day-light behavior and storms, meteors and radiation. In light of these considerations, we chose the Valles Marineris
canyon system as the optimal location. Located in proximity to the equator means minimal fluctuation in temperature. The 7 KM deep
canyon provides a thicker atmosphere and the canyon walls acts as additional protection from the elements.
Reliability testing of the habitat will be in three extreme Earth environments, to simulate the climate on Mars. These places were
chosen due to their climate profile and fluctuation, presence of dust storms, scarcity of water and terrain makeup.
7. Fiber optics detail Water tank from above
Sanitation separate from food for good health
Research area near door to minimize the spread of dust
Sleeping area doesn’t face public functions to provide privacy
No wall between living room and kitchen to increase social life
LAYOUTINTERIORINFASTRUCTURE
Furniture and internal walls are built
into the pre-fab bubble
Supports inserted into bubble shell
The same techniques
used to make Bubba
can be used to make
furniture, like me!
Water
Electric
Light
Heat
Take that
MTV cribs!
Function
over
form!
Moving
partitions
Sintered sand
construction
elements
8
The bubble incorporates
. dynamic partitions, providing
the ability to open and close sections
based on social or pragmatic needs. The
layout is based on functional needs.
The overall shape of the bubble is a round dome. This shape was chosen for its energy efficiency. A sphere is the most
. energy efficient shape for a home because it minimizes the face surface of the envelope of the building, that interacts with
its surroundings. The bubble incorporates moving partitions, built in furniture and a plethora of infrastructural solutions. The dynamic
partitions prevent “stir craziness” in the astronauts by allowing their space to change over time. Additionally, it allows for compart-
mentalization, should part of the habitat become compromised.
As structural complexity of
. the prefabricated bubble is
figuratively endless, many internal
structures can be incorporated in its
shape and be ready for use once the
bubble is inflated. For instance,
built-in chairs, tables, work stations
and storage nooks.
The bubble is
. intended to be
quickly integrated
with external
systems and lead
their supply into the
habitat through
prefabricated
channels.
Solar energy in the
. form of light is
collected from external panels
brought through an optical
fiber into a main inlet, from
where it is distributed through
successive optical fibers
throughout the internal living
space.
The same
. optical
fiber system may
be used to create
heatthat can be
used for activating
a small scale 3D
printer, among
other uses.
The bubble
. contains
additional inlets
and distributing
systems for water
and electricity,
which are also
collected through
external units.
8. WATER PIPING ECLSS LOCATION
STATIC WALL CIRCULATION
HIGH SOUND LEVELS
1:150
DYNAMIC WALL
MEDIUM SOUND LEVELS
LOW SOUND LEVELS
ROOM FUNCTION
SIZE (m²)
9
KITCHEN &
LIVING ROOM
RESEARCH
BATH
FITNESS
BEDROOM
BEDROOM
BEDROOM
BEDROOM
STUDY
BATH