The document discusses the seasons of the Earth. It begins with an introduction to sea breezes and land breezes. It then covers a lesson on the seasons, including a video explaining how the Earth's tilt and revolution around the sun cause the seasons in the Northern and Southern Hemispheres. Students participate in hands-on activities using models of the Earth to illustrate how its axis and movement result in different seasons. They also complete tables to demonstrate their understanding. The importance of understanding seasons and the passage of time is emphasized.
Evolution (Educación Secundaria - Bachillerato - School of stars - Pamploneta...Planetario de Pamplona
Secundaria (3º y 4º), Bachillerato, EPA, CIP. Talleres...
Following the footsteps of two of the most important historical figures in science, Galileo and Darwin, we explore the concept of Evolution in two very different fields: the Universe itself and the life that has developed on Earth.
escuela.pamplonetario.org
George Watts Montessori School Edible Garden Primary Lessons for Classroom & Garden
`
For more information, Please see websites below:
`
Organic Edible Schoolyards & Gardening with Children
http://scribd.com/doc/239851214
`
Double Food Production from your School Garden with Organic Tech
http://scribd.com/doc/239851079
`
Free School Gardening Art Posters
http://scribd.com/doc/239851159`
`
Companion Planting Increases Food Production from School Gardens
http://scribd.com/doc/239851159
`
Healthy Foods Dramatically Improves Student Academic Success
http://scribd.com/doc/239851348
`
City Chickens for your Organic School Garden
http://scribd.com/doc/239850440
`
Simple Square Foot Gardening for Schools - Teacher Guide
http://scribd.com/doc/239851110
do you want an interactive slides which are that you search for grade 6 , 7, 8 level pupils, then it is here. this is readily presentable in a simple language. contains lots real images of moon's phase. the presentatation starts with little introduction consist of pre study about the moon and push students into the content . here you can find attractive animations and images. and also you can find handson experiments and acticities to boost student's interest on this subject. hope you people will enjoy
Interactive , informative and capitivating presentation on phases of moon. Help the listener to easily grasp the concept with more pictures and animations. You can use presentation to teach students of class 6, 7 and 8.
Started with brief introduction which is more informative. Checks the prestudy required. Then move into the content which need to be explained. Explained clearly about eight phases of moon with actual images . additionally explained with images representing positions of sun moon and earth.
Seasons refer to the four different periods of the year, each characterized by distinctive weather patterns and environmental changes. The four seasons are spring, summer, fall (also known as autumn), and winter. The changing of seasons is caused by the Earth's axial tilt and its revolution around the sun.
During each season, different parts of the world experience different weather conditions, such as varying temperatures, precipitation, and daylight hours. For example, in the northern hemisphere, winter is characterized by colder temperatures and shorter daylight hours, while summer is marked by warmer temperatures and longer days.
The changing of seasons has significant impacts on various aspects of life, including agriculture, tourism, and wildlife. Additionally, different cultures and traditions have developed around the seasons, with many holidays and celebrations occurring during specific times of the year.
Overall, understanding the seasons is important for gaining a better appreciation of the natural world and how it affects our lives.
Teacher training presentation used during Universe in the Classroom phase 1 (2014-2015). Covers the following topics: Moon, Earth, Sun, Solar System and Constellations using the Universe-in-a-Box hands-on toolkit.
Evolution (Educación Secundaria - Bachillerato - School of stars - Pamploneta...Planetario de Pamplona
Secundaria (3º y 4º), Bachillerato, EPA, CIP. Talleres...
Following the footsteps of two of the most important historical figures in science, Galileo and Darwin, we explore the concept of Evolution in two very different fields: the Universe itself and the life that has developed on Earth.
escuela.pamplonetario.org
George Watts Montessori School Edible Garden Primary Lessons for Classroom & Garden
`
For more information, Please see websites below:
`
Organic Edible Schoolyards & Gardening with Children
http://scribd.com/doc/239851214
`
Double Food Production from your School Garden with Organic Tech
http://scribd.com/doc/239851079
`
Free School Gardening Art Posters
http://scribd.com/doc/239851159`
`
Companion Planting Increases Food Production from School Gardens
http://scribd.com/doc/239851159
`
Healthy Foods Dramatically Improves Student Academic Success
http://scribd.com/doc/239851348
`
City Chickens for your Organic School Garden
http://scribd.com/doc/239850440
`
Simple Square Foot Gardening for Schools - Teacher Guide
http://scribd.com/doc/239851110
do you want an interactive slides which are that you search for grade 6 , 7, 8 level pupils, then it is here. this is readily presentable in a simple language. contains lots real images of moon's phase. the presentatation starts with little introduction consist of pre study about the moon and push students into the content . here you can find attractive animations and images. and also you can find handson experiments and acticities to boost student's interest on this subject. hope you people will enjoy
Interactive , informative and capitivating presentation on phases of moon. Help the listener to easily grasp the concept with more pictures and animations. You can use presentation to teach students of class 6, 7 and 8.
Started with brief introduction which is more informative. Checks the prestudy required. Then move into the content which need to be explained. Explained clearly about eight phases of moon with actual images . additionally explained with images representing positions of sun moon and earth.
Seasons refer to the four different periods of the year, each characterized by distinctive weather patterns and environmental changes. The four seasons are spring, summer, fall (also known as autumn), and winter. The changing of seasons is caused by the Earth's axial tilt and its revolution around the sun.
During each season, different parts of the world experience different weather conditions, such as varying temperatures, precipitation, and daylight hours. For example, in the northern hemisphere, winter is characterized by colder temperatures and shorter daylight hours, while summer is marked by warmer temperatures and longer days.
The changing of seasons has significant impacts on various aspects of life, including agriculture, tourism, and wildlife. Additionally, different cultures and traditions have developed around the seasons, with many holidays and celebrations occurring during specific times of the year.
Overall, understanding the seasons is important for gaining a better appreciation of the natural world and how it affects our lives.
Teacher training presentation used during Universe in the Classroom phase 1 (2014-2015). Covers the following topics: Moon, Earth, Sun, Solar System and Constellations using the Universe-in-a-Box hands-on toolkit.
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.
Richard's aventures in two entangled wonderlandsRichard 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.
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.
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.
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.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
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.
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.
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/
4. 1. In a __________, the air is warmer above the land.
ASE REEBZE
SEA BREEZE
5. 2. In a land breeze, the air moves from the land to the
__________.
CEOAN
OCEAN
6. 3. In a sea breeze, the air moves from the ocean to the
__________.
NALD
LAND
7. 4. When warm air rises, __________ pressure forms at the
surface of the land or sea.
WOL
LOW
8. 5. The strength of the sea breeze depends on the
difference between __________ of the sea and the land.
PETMERTUARE
TEMPERATURE
9. Questions:
• How do you differentiate a Sea Breeze and a Land Breeze?
• Why do we need to learn about Monsoons?
• Discuss briefly why clouds are densely formed near the Earth’s Equator.
Very good, students!
So, now you have already explored the occurrence of common atmospheric
phenomena and how these provide clear understanding of the Earth we are in.
It also gives us information on how to plan our daily activities based on daily
weather forecast we see and hear on televisions and radios.
Let’s move on to our new lesson for today. But before that, I want you to pay
attention and observe this video.
Present the video Kanlungan.
10. Questions:
• What is the song all about?
• What can you say about the pictures presented in the video? What does it
show?
• Do you still experience or do those things to this day? Why or why not?
That’s right!
So, based on the lyrics of the song “pana-panahon ang pagkakataon”, our
experiences before as a kid is very different from our experiences nowadays
specially that we are already in the gadgets and internet era that is because of
CHANGE. As the saying goes, “Change is the only constant in this world.” Do
you agree? Very good!
Our lesson for today has something to do with the passage of time or
change. Therefore, I want you guys to listen very carefully because today we’re
going to learn about…
12. Target Goals
• identify the different seasons of the Earth
• create a model showing the Earth moving around the sun in
different times of the year
• draw and label the seasons in each hemisphere of the Earth
• discuss the importance of the passage of time and change
13. Have you experience sometimes na it’s already past 6:00 in the evening and
yet hayag gihapon kaayo? Or maybe sometimes it’s already 5:00 in the morning
but then ngitngit gihapon kayo ang kabuntagon.
So the length of days and nights vary. There are times when the days are
longer and the nights are shorter while there are periods during the year when
the nights become longer and the days shorter. Why is this so? What is the
effect of this to the seasons of the Earth?
Let’s all find out as we go along with this lesson.
Yesterday I asked you to prepare certain materials you can find at home for
our activity today. Did you have that one? Kindly put them now on your table.
Please make sure that it is safe enough for you to use the candle if you are
using one. Siguradohon nga secure ang stand sa candle.
Are you ready? This time, let’s create a model showing the Earth moving
around the sun in different times of the year by following this procedures.
14. Procedures:
1. Make an actual model by using a
ball or any round object to
represent the Earth and a
flashlight or a lighted candle to
represent the Sun.
2. Draw a line at the center of the
ball to represent the Equator.
3. Mark “N” for North Pole on top of
the ball and “S” for South Pole at
the bottom of the ball.
15. Procedures:
4. Make sure to move the ball in slanting
position around the lighted candle or
bulb.
5. Make sure to keep the ball at the same
angle as you move it to the other side of
the lighted bulb or candle since the
Earth’s axis is in slanting position which
is about 23.5 degrees from a line
standing to its orbit. Observe also at what
hemisphere the light of the candle
brightens most on the different months.
16. In Araling Panlipunan, in your elementary days you learned that there are
imaginary lines on the globe. This includes horizontal and vertical lines. The
vertical line is what we call longitude and its starting point is called Prime
Meridian. The Prime Meridian divides the Western and Eastern hemisphere of the
Earth. The horizontal line, on the other hand, is called latitude and its starting
point is called the equator. The equator divides the Northern and Southern
hemisphere of the Earth.
Now there are still four other lines parallel to the equator in the northern and
southern hemisphere. What are these lines?
That’s correct! Why are these lines significant for us to know when we talk
about seasons of the Earth?
Very good! And aside from that, these lines help in identifying and locating
major heat zones of the earth. Which means, through these lines, mahibaluan
nato which places on Earth receives direct rays from the sun or not which
ultimately gives us the idea of what season these places are exactly experiencing.
Going back to our activity…
17. Questions:
• In which month is the North Pole tilted toward the Sun – in June or
December?
• In which month is the North Pole tilted away from the Sun – in June or
December?
• In June, which hemisphere receives direct rays from the Sun – the
Northern Hemisphere or Southern Hemisphere?
• In December, which hemisphere receives direct rays from the Sun –
the Northern Hemisphere or Southern Hemisphere?
So, you are going to answer these questions through the next activity
that I am going to show you.
18. Activity: Complete Me
Directions: Use your model as your reference in answering Table 1. Copy and complete the table
below by putting a check mark (✓) in the appropriate column.
19. How do you find the activity? Let’s set that aside in the mean time and I
want you guys to direct your attention on the screen for this short video
lesson. Follow up activities will be done shortly after this to test your
understanding so please make sure to listen very carefully.
Present video lesson about Seasons of the Earth.
20. Summer Solstice
• Longer days, shorter nights
• 90 degrees in Northern
Hemisphere
Winter Solstice
• Shorter days, longer nights
• 90 degrees in Southern
Hemisphere
Spring/Fall Equinox
• Equal day and night
• 90 degrees at equator
WINTER
SPRING
SUMMER
FALL
23. • Direct rays mean that the rays of the
Sun hit the ground at 90 degrees.
• When the Sun’s rays strike the
ground at a high angle, each square
meter of the ground receives a
greater amount of solar energy
which results to a warmer
environment.
• When the Sun’s rays come in at an
oblique angle, each square meter of
the ground will receive a lesser
amount of solar energy because it
will be distributed over a wider area.
27. Activity: Draw & Label Me
Directions:
Copy and complete the diagram below
to illustrate the changes in seasons.
Using the model below as a starting
point:
1. draw the axis on each Earth (E) at
different time of the year;
2. label the seasons in each
hemisphere; and
3. describe the tilt of the Earth and the
seasons.
28.
29. Think-Alone-Share:
• Differentiate rotation and revolution.
• How do you define seasons?
• Enumerate the four (4) seasons on Earth and explain why they happen.
• Why do we experience wet and dry seasons in the Philippines unlike other
countries?
• How important is it to be knowledgeable about seasons and the passage of
time?
Very good, students! You have really understood our lesson well. I am so
happy that not only did the girls participate but as well as the boys. But we’re
not quite done yet because you are still going to answer the Assessment Test
through Quizziz. So I’m going to send you the link and then for 15 minutes, you
are going to answer the quiz.
30. Assignment
Directions: Copy and complete Table 4 by putting a check mark (✓) on the appropriate column. Use
the data in Table 3 below which shows the times of sunrise and sunset in every 22nd day
of the month as your reference. (The first column is done for you.)