Uranus is a gas giant planet with an atmosphere composed primarily of hydrogen and helium. Unlike the other planets in the solar system, Uranus spins on its side due to a large collision in the past. Uranus has 27 known moons named after characters from Shakespearean plays. The planet is extremely cold with an average temperature of -224 degrees Celsius due to its composition and distance from the Sun. It has a system of faint rings and weather characterized by powerful winds and storms.
Maybe too in-depth for most elementary students, but very good broad coverage for teacher background or more advanced students in elementary or middle school.
Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn is named after the Roman god Saturn, equated to the Greek Cronus (the Titan father of Zeus), the Babylonian Ninurta and the Hindu Shani.
A PowerPoint presentation designed for 5th graders that teaches facts about Mercury, including the Mariner 10 and MESSENGER probes that NASA sent to study it. This is Part 1 of the inner planets.
Maybe too in-depth for most elementary students, but very good broad coverage for teacher background or more advanced students in elementary or middle school.
Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn is named after the Roman god Saturn, equated to the Greek Cronus (the Titan father of Zeus), the Babylonian Ninurta and the Hindu Shani.
A PowerPoint presentation designed for 5th graders that teaches facts about Mercury, including the Mariner 10 and MESSENGER probes that NASA sent to study it. This is Part 1 of the inner planets.
This PowerPoint is one small part of the Astronomy Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 3000+ slide PowerPoint roadmap, 12 page bundled homework package, modified homework, detailed answer keys, 8 pages of unit notes for students who may require assistance, follow along worksheets, and many review games. The homework and lesson notes chronologically follow the PowerPoint slideshow. The answer keys and unit notes are great for support professionals. The activities and discussion questions in the slideshow and meaningful. The PowerPoint includes built-in instructions, visuals, and follow up questions. Also included are critical class notes (color coded red), project ideas, video links, and review games. This unit also includes four PowerPoint review games (110+ slides each with Answers), 38+ video links, lab handouts, activity sheets, rubrics, materials list, templates, guides, and much more. Also included is a 190 slide first day of school PowerPoint presentation. Teaching Duration = 5+ weeks. Areas of Focus in the Astronomy Topics Unit: The Solar System and the Sun, Order of the Planets, Our Sun, Life Cycle of a Star, Size of Stars, Solar Eclipse, Lunar Eclipse, The Inner Planets, Mercury, Venus, Earth, Moon, Craters, Tides, Phases of the Moon, Mars and Moons, Rocketry, Asteroid Belt, NEOs, The Torino Scale, The Outer Planets and Gas Giants, Jupiter / Moons, Saturn / Moons, Uranus / Moons, Neptune / Moons, Pluto's Demotion, The Kuiper Belt, Oort Cloud, Comets / Other, Beyond the Solar System, Types of Galaxies, Blackholes, Extrasolar Planets, The Big Bang, Dark Matter, Dark Energy, The Special Theory of Relativity, Hubble Space Telescope, Constellations, Spacetime and much more. If you have any questions please feel free to contact me. Thanks again and best wishes. Sincerely, Ryan Murphy M.Ed www.sciencepowerpoint@gmail.com
The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)Fatimah Sol Jalmaani
We did last year (2012), with my classmates Gloriele and Abegail for a report. Anyone can get information from it, but if you plan to use ALL OF IT, make sure to site the source, okay????! That's all! :D
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...Ana Luísa Pinho
Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
2. The Planet
Like Jupiter and Saturn, Uranus is a gas giant. But Uranus
is a little different. Unlike all the other planets and most of
the moons in our Solar System, Uranus spins on its side. It
is believed that long ago a very large object smashed into
this planet. The crash was so powerful that it completely
changed the direction of Uranus' planetary rotation.
However, a more recent theory is that the extreme tilt of
Uranus' axis may have been caused by a large moon that
was slowly pulled away from the planet by another large
planet long ago when our Solar System was still new.
3. History
• William Herschel discovered Uranus on
March 13, 1781.
• Uranus was named after the Greek god
deity who was the god of the sky
• This is Uranus's symbol
4. Solar System
• Uranus is the 7th
planet from the sun.
Uranus is 1,787,485,510 miles (2,876,679,082 km) away from the sun
• It takes Uranus 84 years to circle around the sun
• Below is a picture showing Uranus's relationship in space to other
planets.
5. Uranus's Measurements
• Uranus is the third largest planet in the solar system, after Jupiter
and Saturn. Uranus is about four times bigger than Earth. Its
diameter at the equator is about 31,763 miles 51,118 kilometers as
measured at the level of the atmosphere where the pressure is the
same as at sea level on Earth. The planet is slightly larger than
Neptune but Neptune is about 1.2 times more massive. Uranus's'
density is quite low only about 1.3 times that of water, compared
with 1.6 for Neptune and 5.5 for Earth.
• Mass - Metric: 86,810,300,000,000,000,000,000,000 kg
Volume- metric- 68,334,355,695,584 km3
• Surface Gravity Metric: 8.87 m/s2
• Orbit Circumference Metric: 18,026,802,831 km
6. The atmosphere and core of
Uranus
• Uranus is shrouded in an icy cloud layer made up of
frozen methane, ethane, and acetylene circling this
planet at about 185 mph (300 kph. Uranus' icy and cold
atmosphere consist of 83% hydrogen,15% helium, and
2% methane.
• Uranus has a molten rocky core about 10,500 miles
(17,000 km) in diameter and about 12,500°F (6927°C).
This core may have a mass five times greater than the
mass of the Earth.
7. Surface Conditions or Uranus
• Uranus is not the farthest planet from the
Sun but it is the coldest planet in the Solar
System.
• The average temperature of the surface of
Uranus is 49° Kelvin or -224° Celsius.
• Uranus is so cold because its core.Uranus
is only 5000° K, compared to Jupiter,
which as a core temperature of 30000° K.
8. Moons
• Uranus has 27 named after characters from the works of
William Shakespeare and Alexander Pope. Scientists
believe that Uranus has more than 30 moons but they have
not been discovered yet
• Moon names
• Caliban, Stephano, Trinculo, Sycorax, Margaret, Prospero,
Setebos, Mab, Pertida, Cupid, Francisco, Ferdinand,
Oberon, Titania, Umbriel, Ariel, Miranda, Puck, Rosalind
Portia, Juliet ,Desdemona ,Cressida, Bianca ,Ophelia and
Cordelia.
9. Rings
• Uranus has different rings than Jupiter and Saturn.
Uranus's rings are very small and spaced out so it looks
like there are several skinny rings with big gaps in-
between.
• Astronomers think that the rings of Uranus are very
young, and probably formed recently, and not with the
planet.
10. Please watch this amazing
video on Uranus
click below
•Click the picture
11. What would happen if a human
went to Uranus?
If a human went on Uranus they would freeze because of
the low temperatures on Uranus. A human would also
choke because the extremely low oxygen levels. In order to
explore Uranus safely a human would need an oxygen tank
and a body warmer along with probably 200 winter coats.
12. Fun facts
• If you way 100 pounds on earth you will weight
91 pounds on Uranus.
• It will take 141/2
earths to fill Uranus
• Summer on Uranus lasts 42 years.
• Uranus was the first planet discovered in the
modern age.
• A day on Uranus is 17 hours, 14 minutes
and 24 seconds.
13.
14. Weather on Uranus
• Here’s the scoop about weather on Uranus. A thick,
tempestuous atmosphere with winds blowing at a clip of
560 mph; massive storms that would engulf continents
here on Earth, and temperatures in the -220 degrees
Celsius -360 degree Fahrenheit