Galaxy is a system of millions or billions of stars held together by gravity. There are three main types of galaxies: irregular galaxies with an irregular shape resulting from galaxy collisions, elliptical galaxies with little structure or rotation, and spiral galaxies with a central hub and spiral arms promoting star formation.
The Milky Way is a barred spiral galaxy containing our solar system. It is named for its hazy, milky appearance in the night sky. The Milky Way is part of a group of galaxies called the Local Group within the larger Virgo Supercluster.
A GENERAL OVERVIEW OF THE PLANET JUPITER INCLUDING ITS COMPONENTS
A REPORT CREATED BY STUDENTS OF SAINT CATHERINE'S SCHOOL
BAMBANG, NUEVA VIZCAYA
CREDITS TO THE OWNERS OF THE REPORT:
Jan Phillip Gamponia
Jolina Mae Valdez
Lady Erika Fernandez
Ronnrick Manuel
Roxanne Hangdaan
Astronomy is known as the science of the entire universe beyond the Earth. It includes the Earth’s gross physical properties: its mass and rotation, as they interact with other bodies of the solar system.
A GENERAL OVERVIEW OF THE PLANET JUPITER INCLUDING ITS COMPONENTS
A REPORT CREATED BY STUDENTS OF SAINT CATHERINE'S SCHOOL
BAMBANG, NUEVA VIZCAYA
CREDITS TO THE OWNERS OF THE REPORT:
Jan Phillip Gamponia
Jolina Mae Valdez
Lady Erika Fernandez
Ronnrick Manuel
Roxanne Hangdaan
Astronomy is known as the science of the entire universe beyond the Earth. It includes the Earth’s gross physical properties: its mass and rotation, as they interact with other bodies of the solar system.
What is a solar system?
FORMATION OF SOLAR SYSTEM
Components of the SOLAR SYSTEM
Discovery and exploration
Terminology
Description of the Components of the SOLAR SYSTEM
Farthest Regions
Galactic Context
The Solar System is located in the Milky Way galaxy, a barred spiral galaxy with a diameter of about 100,000 light-years containing about 200 billion stars. Our Sun resides in one of the Milky Way's outer spiral arms, known as the Orion Arm or Local Spur. The Sun lies between 25,000 and 28,000 light years from the Galactic Centre, and its speed within the galaxy is about 220 kilometres per second, so that it completes one revolution every 225–250 million years. This revolution is known as the Solar System's galactic year. The solar apex, the direction of the Sun's path through interstellar space, is near the constellation of Hercules in the direction of the current location of the bright star Vega. The plane of the Solar System's ecliptic lies nearly at right angles (86.5°) to the galactic plane.
What is a solar system?
FORMATION OF SOLAR SYSTEM
Components of the SOLAR SYSTEM
Discovery and exploration
Terminology
Description of the Components of the SOLAR SYSTEM
Farthest Regions
Galactic Context
The Solar System is located in the Milky Way galaxy, a barred spiral galaxy with a diameter of about 100,000 light-years containing about 200 billion stars. Our Sun resides in one of the Milky Way's outer spiral arms, known as the Orion Arm or Local Spur. The Sun lies between 25,000 and 28,000 light years from the Galactic Centre, and its speed within the galaxy is about 220 kilometres per second, so that it completes one revolution every 225–250 million years. This revolution is known as the Solar System's galactic year. The solar apex, the direction of the Sun's path through interstellar space, is near the constellation of Hercules in the direction of the current location of the bright star Vega. The plane of the Solar System's ecliptic lies nearly at right angles (86.5°) to the galactic plane.
This unit has been designed to support Year 3 teachers. It integrates some of the Primary Connections Ideas and acknowledges these, yet also add additional resources. We have tried to incorporate higher order thinking skills within the unit.
If you like this resource like and share http://www.australiancurriculumlessons.com.au/2014/08/09/earth-moon-sun-lessons-plans-year-34/ (I am trying to win my son an iPad. The resource on this site with the most likes wins an iPad Mini).
Power Point notes that I use in class. I did not make this presentation. I got it from the internet, the reference is on the first page. I may have altered it from it\'s origninal state though.
The Milky Way Galaxy and The types of exoplanets.pdfClaireTan46
For Educational purposes only. All credits for the image and facts goes to the original creators. I'm just sharing it here to express the beauty and inspiration of the universe and the amazing potential for human connection that lies within it.
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.
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.
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.
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...Scintica Instrumentation
Intravital microscopy (IVM) is a powerful tool utilized to study cellular behavior over time and space in vivo. Much of our understanding of cell biology has been accomplished using various in vitro and ex vivo methods; however, these studies do not necessarily reflect the natural dynamics of biological processes. Unlike traditional cell culture or fixed tissue imaging, IVM allows for the ultra-fast high-resolution imaging of cellular processes over time and space and were studied in its natural environment. Real-time visualization of biological processes in the context of an intact organism helps maintain physiological relevance and provide insights into the progression of disease, response to treatments or developmental processes.
In this webinar we give an overview of advanced applications of the IVM system in preclinical research. IVIM technology is a provider of all-in-one intravital microscopy systems and solutions optimized for in vivo imaging of live animal models at sub-micron resolution. The system’s unique features and user-friendly software enables researchers to probe fast dynamic biological processes such as immune cell tracking, cell-cell interaction as well as vascularization and tumor metastasis with exceptional detail. This webinar will also give an overview of IVM being utilized in drug development, offering a view into the intricate interaction between drugs/nanoparticles and tissues in vivo and allows for the evaluation of therapeutic intervention in a variety of tissues and organs. This interdisciplinary collaboration continues to drive the advancements of novel therapeutic strategies.
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.
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.
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.
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.
2. What is Galaxy?
Galaxy is a system of millions or billions of stars, together with
gas and dust, held together by gravitational attraction.
The word galaxy is derived from the Greek galaxias literally
"milky", a reference to the Milky Way.
3.
4. These galaxies have an irregular
shape and are considered to be
the result of the collisions
galaxies. As a result, they
generally contain of a complex
mix of interstellar gas and dust,
young stars, and old stars.
Irregular
5. These galaxies have little to no
structure, rotation, or
interstellar matter. This results
in minimal tar formation and a
dominance of the long lived,
red stars. These ellipsoid-
shaped collection of stars are
the most common type of
galaxy.
6. These galaxies are disk-shaped
with either a round central hub
(unbarred) or a hub shaped
like a bar (barred). They rotate
with spiral arms that contain
interstellar dust and gas,
promoting star formation and
an abundance of young stars.
8. What is Milky Way?
It is the name of the barred spiral galaxy in which our solar system is located. The
Earth orbits the Sun in the Solar System, and the Solar System is embedded within
this vast galaxy of stars. It is just one of hundreds of billions of galaxies in the
Universe, and ours is called the Milky Way because the disk of the galaxy appears to
be spanning the night sky like a hazy band of glowing white light.
In short, our galaxy was named because of the way the haze it casts in the night sky
resembled spilled milk. This name is also quite ancient. It is translation from the
Latin “Via Lactea“, which in turn was translated from the Greek for Galaxias,
referring to the pale band of light formed by stars in the galactic plane as seen from
Earth.
9. The Milky Way is part of a collection of galaxies called the Local Group.
The Milky Way is the galaxy that contains our Solar System. Its name "milky" is
derived from its appearance as a dim glowing band arching across the night sky
whose individual stars cannot be distinguished by the naked eye. T
The ancient Romans called our galaxy the Via Lactea, which literally means “The
Road of Milk.”
The Milky Way is the second-largest galaxy.
Notice that the total size of the Milky Way is about 50,000 light-years in radius,
with the Sun a little over halfway from the center.
The Milky Way contains between 100- 400 billion stars and at least 100 billion
planets
11. The Milky Way and the
Andromeda Galaxy are a
binary system of giant spiral
galaxies belonging to a
group of 50 closely bound
galaxies known as the Local
Group, itself being part of
the Virgo Supercluster.
13. The "Milky Way" can be seen as a
hazy band of white light some 30
degrees wide arcing across the sky.
The area of the sky obscured by the
Milky Way is called the Zone of
Avoidance.
14. The Milky Way consists of a bar-shaped core region
surrounded by a disk of gas, dust and stars. The gas,
dust and stars are organized in roughly logarithmic
spiral arm structures
15.
16. The Milky Way began as one or several small over
densities in the mass distribution in the Universe
shortly after the Big Bang. Some of these over
densities were the seeds of globular clusters in
which the oldest remaining stars in what is now
the Milky Way formed.
17. Globular clusters are among the
oldest objects in the Milky Way,
which thus set a lower limit on the
age of the Milky Way. The ages of
individual stars in the Milky Way can
be estimated by measuring the
abundance of long-lived radioactive
elements such as thorium-232 and
uranium-238, then comparing the
results to estimates of their original
abundance, a technique called
nucleocosmochronology.
Age
18. Our Sun is located in the Orion Arm,
a region of space in between the two
major arms of the Milky Way, and
about 27,000 light years from the
galactic core. At the heart of the
Milky Way is a super-massive black
hole, just like all of the other
galaxies, known as Sagittarius A*.
This monster is more than 4 million
times the mass of the Sun and is
believed to have a diameter of 44
million kilometers.