The document summarizes key information about the solar system, including its composition of planets, moons, asteroids, and comets. It lists the nine major planets - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. Details are provided about each planet's characteristics such as size, distance from the sun, surface features, temperatures, and chemical makeup. Additional facts about moons, rings, and material in the solar system are mentioned.
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THIS ABOUT SUN . SLIDE PRESENTATION
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THIS ABOUT SUN . SLIDE PRESENTATION
Our solar system consists of our star, the Sun, and everything bound to it by gravity — the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune, dwarf planets such as Pluto, dozens of moons and millions of asteroids, comets and meteoroids.
Presentación power point de los planetas interiores, realizada por dos alumnas de bachillerato, que tienen un blog en común para la asignatura de ciencias para el mundo contemporáneo.
Presentation on Solar System for primary level students.
Solar system is the collection of eight planets and their moons in orbit round the sun, together with smaller bodies in the form of asteroids, meteoroids, and comets.
Our solar system consists of our star, the Sun, and everything bound to it by gravity — the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune, dwarf planets such as Pluto, dozens of moons and millions of asteroids, comets and meteoroids.
Presentación power point de los planetas interiores, realizada por dos alumnas de bachillerato, que tienen un blog en común para la asignatura de ciencias para el mundo contemporáneo.
Presentation on Solar System for primary level students.
Solar system is the collection of eight planets and their moons in orbit round the sun, together with smaller bodies in the form of asteroids, meteoroids, and comets.
1. The Sun: The Sun is a G-type main-sequence star, which means it is a relatively stable, middle-aged star. It makes up about 99.86% of the Solar System's total mass. The Sun is composed mainly of hydrogen (about 74% by mass) and helium (about 24% by mass), with traces of other elements. It is the source of light and energy for the entire Solar System through nuclear fusion in its core. The Sun has a diameter of about 1.4 million kilometers (870,000 miles) and a mass approximately 333,000 times that of Earth. It has a surface temperature of around 5,500 degrees Celsius (9,932 degrees Fahrenheit) and is about 4.6 billion years old. The Sun's gravitational influence keeps the planets of the solar system in orbit around it, and its solar wind extends far beyond the orbit of Pluto, defining the heliosphere
2. Inner Planets (Terrestrial Planets)
Outer Planets (Gas Giants)
Dwarf Planets and Trans-Neptunian Objects (TNOs)
Galaxies
Galaxies are vast systems that consist of stars, stellar remnants, interstellar gas, dust, and dark matter, all bound together by gravity. They are the fundamental building blocks of the universe, and their study provides crucial insights into the structure, composition, and evolution of the cosmos.
Types of Galaxies
1. Elliptical Galaxies: Elliptical, ranging from nearly spherical (E0) to highly elongated (E7). Comprised mainly of older stars, with little interstellar gas and dust. Generally, lack ongoing star formation and are often found in galaxy clusters.
2. Spiral Galaxies: Contain a mix of old and young stars, along with significant amounts of gas and dust. Ongoing star formation in the spiral arms, and they often have a rotating disk structure.
3. Irregular Galaxies: Lack a distinct regular structure. Varied mix of young and old stars, as well as gas and dust. Often the result of gravitational interactions or mergers between galaxies.
Milky Way Galaxy:
- The Milky Way is the barred spiral galaxy that includes our solar system.
- It has a central bar-shaped structure with spiral arms extending outward.
- The Milky Way is part of the Local Group, a collection of galaxies that also includes the Andromeda Galaxy and many smaller galaxies.
Galaxy Clusters:
- Galaxies are not randomly distributed; they often form groups and clusters.
- Galaxy clusters are massive structures containing hundreds or thousands of galaxies bound together by gravity.
- The Virgo Cluster is one of the closest galaxy clusters to the Milky Way.
Galaxy Formation and Evolution:
- Galaxies form through the gravitational collapse of gas and dark matter.
- Interactions between galaxies, such as mergers, can significantly impact their structure and star formation.
- Galaxies evolve over time, with factors like star formation, supernova explosions, and feedback from supermassive black holes playing key roles.
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
This pdf is about the Schizophrenia.
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Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
Richard's entangled aventures in wonderlandRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Slide 1: Title Slide
Extrachromosomal Inheritance
Slide 2: Introduction to Extrachromosomal Inheritance
Definition: Extrachromosomal inheritance refers to the transmission of genetic material that is not found within the nucleus.
Key Components: Involves genes located in mitochondria, chloroplasts, and plasmids.
Slide 3: Mitochondrial Inheritance
Mitochondria: Organelles responsible for energy production.
Mitochondrial DNA (mtDNA): Circular DNA molecule found in mitochondria.
Inheritance Pattern: Maternally inherited, meaning it is passed from mothers to all their offspring.
Diseases: Examples include Leber’s hereditary optic neuropathy (LHON) and mitochondrial myopathy.
Slide 4: Chloroplast Inheritance
Chloroplasts: Organelles responsible for photosynthesis in plants.
Chloroplast DNA (cpDNA): Circular DNA molecule found in chloroplasts.
Inheritance Pattern: Often maternally inherited in most plants, but can vary in some species.
Examples: Variegation in plants, where leaf color patterns are determined by chloroplast DNA.
Slide 5: Plasmid Inheritance
Plasmids: Small, circular DNA molecules found in bacteria and some eukaryotes.
Features: Can carry antibiotic resistance genes and can be transferred between cells through processes like conjugation.
Significance: Important in biotechnology for gene cloning and genetic engineering.
Slide 6: Mechanisms of Extrachromosomal Inheritance
Non-Mendelian Patterns: Do not follow Mendel’s laws of inheritance.
Cytoplasmic Segregation: During cell division, organelles like mitochondria and chloroplasts are randomly distributed to daughter cells.
Heteroplasmy: Presence of more than one type of organellar genome within a cell, leading to variation in expression.
Slide 7: Examples of Extrachromosomal Inheritance
Four O’clock Plant (Mirabilis jalapa): Shows variegated leaves due to different cpDNA in leaf cells.
Petite Mutants in Yeast: Result from mutations in mitochondrial DNA affecting respiration.
Slide 8: Importance of Extrachromosomal Inheritance
Evolution: Provides insight into the evolution of eukaryotic cells.
Medicine: Understanding mitochondrial inheritance helps in diagnosing and treating mitochondrial diseases.
Agriculture: Chloroplast inheritance can be used in plant breeding and genetic modification.
Slide 9: Recent Research and Advances
Gene Editing: Techniques like CRISPR-Cas9 are being used to edit mitochondrial and chloroplast DNA.
Therapies: Development of mitochondrial replacement therapy (MRT) for preventing mitochondrial diseases.
Slide 10: Conclusion
Summary: Extrachromosomal inheritance involves the transmission of genetic material outside the nucleus and plays a crucial role in genetics, medicine, and biotechnology.
Future Directions: Continued research and technological advancements hold promise for new treatments and applications.
Slide 11: Questions and Discussion
Invite Audience: Open the floor for any questions or further discussion on the topic.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
This presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
2. The Solar System consists of:The Solar System consists of:
PlanetsPlanets
MoonsMoons
AsteroidsAsteroids
CometsComets
3. PLANETSPLANETS
A planet is a large, round
heavenly body that orbits
a star and shines with light
reflected from the star. We
know of nine planets that
orbit the sun in our solar
system. Since 1992,
astronomers have also
discovered many planets
orbiting other stars. World book
4. What are the nine planets?What are the nine planets?
HINT: My Very Educated Mother Just Sent Us Nine PizzasHINT: My Very Educated Mother Just Sent Us Nine Pizzas
MercuryMercury
VenusVenus
EarthEarth
MarsMars
JupiterJupiter
SaturnSaturn
UranusUranus
NeptuneNeptune
PlutoPluto
5. MERCURYMERCURY
Mer|cu|ry «MUR kyuhr ee», noun.
The smallest planet in the solar system, after
Pluto, and the one nearest to the sun. Its orbit
about the sun takes 88 days to complete, at a
mean distance of almost 36,000,000 miles. Mercury
goes around the sun about four times while the
earth is going around once.
[< Latin Mercurius]
World Book
6. VENUSVENUS
Venus is the sixth largest
planet in the solar system and
the second in distance from
the sun. Venus is the brightest
planet in the solar system and
the one that comes closest to
the earth. World Book
7. EARTHEARTH
Age:Age: At least 4 1/2 billion yearsAt least 4 1/2 billion years
Mass:Mass: 6,600,000,000,000,000,000,000 (6.6 sextillion)6,600,000,000,000,000,000,000 (6.6 sextillion)
tons (6.0 sextillion metric tons).tons (6.0 sextillion metric tons).
Surface features:Surface features: Highest landHighest land—Mount Everest, 29,035—Mount Everest, 29,035
feet (8,850 meters) above sea level.feet (8,850 meters) above sea level. Lowest landLowest land—shore—shore
of Dead Sea, about 1,310 feet (399 meters) below sea).of Dead Sea, about 1,310 feet (399 meters) below sea).
Temperature:Temperature: Highest,Highest, 136 °F (58 °C) at Al Aziziyah,136 °F (58 °C) at Al Aziziyah,
Libya.Libya. Lowest,Lowest, -128.6 °F (-89.6 °C) at Vostok Station in-128.6 °F (-89.6 °C) at Vostok Station in
Antarctica.Antarctica. Average surface temperature,Average surface temperature, 59 °F (15 °C).59 °F (15 °C).
Chemical makeup of the earth's crust (in percent ofChemical makeup of the earth's crust (in percent of
the crust's weight):the crust's weight): oxygen 46.6, silicon 27.7,oxygen 46.6, silicon 27.7,
aluminum 8.1, iron 5.0, calcium 3.6, sodium 2.8,aluminum 8.1, iron 5.0, calcium 3.6, sodium 2.8,
potassium 2.6, magnesium 2.0, and other elementspotassium 2.6, magnesium 2.0, and other elements
totaling 1.6.totaling 1.6.
8. MARSMARS
The Mars Odyssey probe,The Mars Odyssey probe,
shown in this illustrationshown in this illustration
orbiting Mars, foundorbiting Mars, found
evidence of water iceevidence of water ice
beneath the surface ofbeneath the surface of
Mars in 2002. The probe,Mars in 2002. The probe,
launched in 2001, alsolaunched in 2001, also
analyzed the chemicalanalyzed the chemical
composition of thecomposition of the
planet's surface.planet's surface. World BookWorld Book
9. What is this planet called?What is this planet called?
11. JupiterJupiter
JupiterJupiter is the largest planet in the solar system.is the largest planet in the solar system.
Its diameter is 88,846 miles (142,984Its diameter is 88,846 miles (142,984
kilometers), more than 11 times that of Earth,kilometers), more than 11 times that of Earth,
and about one-tenth that of the sun. It wouldand about one-tenth that of the sun. It would
take more than 1,000 Earths to fill up thetake more than 1,000 Earths to fill up the
volume of the giant planet. When viewed fromvolume of the giant planet. When viewed from
Earth, Jupiter appears brighter than most stars.Earth, Jupiter appears brighter than most stars.
It is usually the second brightest planet—afterIt is usually the second brightest planet—after
Venus.Venus.
14. URANUSURANUS
one of the larger planets in the solar system and the seventh in distance from the sun.
U|ra|nus «yu RAY nuhs, YUR uh-», noun.
15. NEPTUNENEPTUNE
LatinLatin ,, relatedrelated
toto nebulanebula
cloud, mistcloud, mist
In Neptune's outermost ring, 39,000 miles
(63,000 kilometers) from the planet, material
mysteriously clumps into three bright, dense
arcs.
NASA
16. PLUTOPLUTO
Is Pluto a planet? Yes, Pluto is a
planet. The body that decides the
classification of objects in the solar
system, the International Astronomical
Union (IAU), has no plans to change
Pluto's status as a planet and has
decided against assigning it a minor
planet number. For more on this
decision, see:
http://www.iau.org/IAU/FAQ/PlutoPR.html.