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GRADE 1 to 12
DAILY LESSON LOG
School Ozamiz City National High School Grade Level Grade 11
Teacher Jerda U. Idio Learning Area Physical Science
Teaching Dates and Time February 5-8, 2024 Quarter 3rd
CLASS SESSION 1 CLASS SESSION 2 CLASS SESSION 3 CLASS SESSION 4
I. OBJECTIVES
Objectives must be met over the week and connected to the curriculum standards. To meet the objectives necessary procedures must be followed and if needed, additional lessons, exercises, and
remedial activities must be done for developing content knowledge and competencies. These are assessed using Formative Assessment strategies. Valuing objectives support the learning of content
and competencies and enable children to find significance and joy in learning the lessons. Weekly objectives shall be derived from the curriculum guides.
A. Content Standards
The learners demonstrate understanding of:
1. the formation of the elements during the Big Bang and during stellar evolution
2. the distribution of the chemical elements and the isotopes in the universe
B. Performance Standards
The learners should be able to:
1. Make a creative representation of the historical development of the atom or the chemical element in a timeline
C. Learning Competencies/Objectives
Write the LC code for each.
 Give evidence for and
describe the formation of
heavier elements during star
formation and evolution
 Give evidence for and
describe the formation of
heavier elements during star
formation and evolution
 Explain how the concept of
atomic number led to the
synthesis of new elements in
the laboratory S11/12PS-IIIb-11
 Explain how the concept of
atomic number led to the
synthesis of new elements in the
laboratory S11/12PS-IIIb-11
D. Objectives
The learners will describe the
formation of heavier elements during
the formation and evolution of stars
The learners will cite astronomical
evidence which justifies the
formation of elements during
stellar formation and evolution
The learners will explain how the
concept of atomic number led to the
synthesis of new elements
The learners will analyse the nuclear
reactions involved in the synthesis of
new elements
II. CONTENT
Content is what the lesson is all about. It pertains to the subject matter that the teacher aims to teach in the CG, the content can be tackled in a week or two.
Formation of Elements During
Stellar Formation and Evolution
Formation of Elements During
Stellar Formation and Evolution
The Synthesis of New Elements The Synthesis of New Elements
III. LEARNING RESOURCES
Let the materials to be used in different days. Varied sources of materials sustain children’s interest in the lesson and in learning. Ensure that there is a mix of concrete and manipulative materials as
well as paper-based materials. Hands-on learning promotes concept development.
A. References
1. Teacher’s Guide pages Physical Science TG Physical Science TG Physical Science TG Physical Science TG
2. Learner’s Materials pages
3. Textbook pages
4. Additional Materials from Learning
Resources (LR) portal
Google/Internet Google/Internet Google/Internet Google/Internet
B. Other Learning Resources
These steps should be done across the week. Spread out the activities appropriately so that students will learn well. Always be guided by demonstration of learning by the students which you can
infer from formative assessment activities. Sustain learning systematically by providing students with multiple ways to learn new things, practice their learning, question their learning processes, and
IV. PROCEDURES draw conclusions about what they learned in relation to their life experiences and previous knowledge. Indicate the time allotment for each step.
A. Reviewing previous lesson or
presenting the new lesson
The teacher will give the overview of
the objectives and key terms for the
quarter.
1. Give a big picture of Chemistry by
describing it as “the study of stuff.”
The teacher will recall the Big Bang
nucleosynthesis and the formation of
lighter
elements.
The teacher will recall the evidences
for and describe the formation of
heavier elements during star
formation and evolution
The teacher will introduce the
following list of important terms that
learners will encounter.
B. Establishing a purpose for the lesson
The teacher will briefly define
cosmology as the study of how the
universe began, how it continues to
exist, and how it will end.
(Offer examples of cosmologies from
different religions and cultures based
on their beliefs)
Guide Question?
1. Do you think there is proof that any
of these stories or cosmologies are
true?
The students will try to refresh your
mind by supplying the number of
protons and neutrons of each
element.
The Cosmic Connection
The teacher will use the Think, Pair,
Share protocol and ask learners to
reflect and share their thoughts on
the selection.
Stellar Word Puzzle!
The learners will encircle and write
down the words which are related to
star and element formation.
C. Presenting examples/instances of the
new lesson
The learners will give important
clues in understanding the
fundamental building blocks of the
universe and how life on earth is
connected to stars.
In the Beginning: The Nebulae!
Guide Questions?
Question 1: Where do you think stars
come from?
The learners will share their insights.
Growing Older, Growing Bigger:
The Red Giant Star!
Guide Questions:
Why do you think red giant stars are
called red giants?
The students will examine the
diagram from your left. It illustrates
an atom’s subatomic particles
namely:
a. protons+
b. neutrons 0
c. electrons _
Activity I.I Making Your Own
Periodic Table
The learners will make their own
periodic table using the hypothetical
elements that are given in the clues.
a. P and Pr both have one electron
each. Pr has a bigger atomic size.
b. Od, Ri, and E are in the same series
as P, C, and I. In terms of atomic
size, P is the biggest while C is the
smallest. E is a metal while I is a
non-metal. Od is smaller than Ri in
atomic size.
D. Discussing new concepts and
practicing new skills # 1
The learners will explore the vast
universe with the countless twinkling
diamonds in the sky.
1.Stars’ Starting Point of Life: The
Protostar!
Guide Questions:
1. What is the core of it all?
The Death of a Star: Depletion of
Energy!
Guide Question:
1. Do you think stars explode when
they die?
The students will determine their
quantity in a certain element
How about isotope 13 Carbon?
protons ____ atomic no.___
neutrons ___ atomic mass__
The learners will write the balanced
nuclear reaction of the following
elements under alpha, beta and
gamma decay.
E. Developing mastery/ Finding practical
applications of concepts and skills in
daily living / Making generalizations
and abstractions about the lesson
Activity 1- “Forget Me Not”
The learners will identify the
following and tell something about
each of them.
Activity 1- “Star in the Making
The learners will demonstrate what
they have learned on the formation
of stars by doing any of the
suggested star projects.
Comic Story- create a one-page comic
star’s life cycle story (cartoons or
cut-outs)
Activity 1-Transformation-
Radiation in One!
The learners will choose the letter of
the symbol that represents the type
of nuclear radiation
Activity 1.1
The learners will write the nuclear
reactions involved in the synthesis of
each of the following new elements:
a. Curium (Z = 96) was formed by
reacting Pu – 239 with alpha
particles 42He. It has a half-life of
162 days.
b. Mendelevium (Z = 101) was formed
by reacting En-253 with alpha
particles.
Rubrics
F. Evaluating learning
Activity 2 – “Twinkle, Twinkle Little
Big Star, How I Wander as You Are!”
The learners will relate the evolution
of a star to the life cycle of a person.
The students will identify the
temperature of each color?
Use this temperature list: 3000 °C,
4500 °C, 6000 °C, 10 000 °C, 40 000
°C
Wrap up!
The learners will answer the
following as you look back at the
things we have talked about today.
1. What is the missing link that led to
the completion of the known
“almost perfect” periodic table of
elements? How did it lead to the
discovery of synthetic elements?
2. How do scientists forge the
synthesis of elements?
3. What happens during the
synthesis of new elements?
The students will create an inventory
list of universe’s fragments into a
systematic compilation that includes
the new synthetic elements
G. Additional activities for application or
remediation
V. REMARKS
Prepared by Checked by
JERDA U. IDIO ALIE A. BONGCAWIL
Subject Teacher Assistant Principal, Senior High Department

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Daily Lesson Log Physical Science week 1

  • 1. GRADE 1 to 12 DAILY LESSON LOG School Ozamiz City National High School Grade Level Grade 11 Teacher Jerda U. Idio Learning Area Physical Science Teaching Dates and Time February 5-8, 2024 Quarter 3rd CLASS SESSION 1 CLASS SESSION 2 CLASS SESSION 3 CLASS SESSION 4 I. OBJECTIVES Objectives must be met over the week and connected to the curriculum standards. To meet the objectives necessary procedures must be followed and if needed, additional lessons, exercises, and remedial activities must be done for developing content knowledge and competencies. These are assessed using Formative Assessment strategies. Valuing objectives support the learning of content and competencies and enable children to find significance and joy in learning the lessons. Weekly objectives shall be derived from the curriculum guides. A. Content Standards The learners demonstrate understanding of: 1. the formation of the elements during the Big Bang and during stellar evolution 2. the distribution of the chemical elements and the isotopes in the universe B. Performance Standards The learners should be able to: 1. Make a creative representation of the historical development of the atom or the chemical element in a timeline C. Learning Competencies/Objectives Write the LC code for each.  Give evidence for and describe the formation of heavier elements during star formation and evolution  Give evidence for and describe the formation of heavier elements during star formation and evolution  Explain how the concept of atomic number led to the synthesis of new elements in the laboratory S11/12PS-IIIb-11  Explain how the concept of atomic number led to the synthesis of new elements in the laboratory S11/12PS-IIIb-11 D. Objectives The learners will describe the formation of heavier elements during the formation and evolution of stars The learners will cite astronomical evidence which justifies the formation of elements during stellar formation and evolution The learners will explain how the concept of atomic number led to the synthesis of new elements The learners will analyse the nuclear reactions involved in the synthesis of new elements II. CONTENT Content is what the lesson is all about. It pertains to the subject matter that the teacher aims to teach in the CG, the content can be tackled in a week or two. Formation of Elements During Stellar Formation and Evolution Formation of Elements During Stellar Formation and Evolution The Synthesis of New Elements The Synthesis of New Elements III. LEARNING RESOURCES Let the materials to be used in different days. Varied sources of materials sustain children’s interest in the lesson and in learning. Ensure that there is a mix of concrete and manipulative materials as well as paper-based materials. Hands-on learning promotes concept development. A. References 1. Teacher’s Guide pages Physical Science TG Physical Science TG Physical Science TG Physical Science TG 2. Learner’s Materials pages 3. Textbook pages 4. Additional Materials from Learning Resources (LR) portal Google/Internet Google/Internet Google/Internet Google/Internet B. Other Learning Resources These steps should be done across the week. Spread out the activities appropriately so that students will learn well. Always be guided by demonstration of learning by the students which you can infer from formative assessment activities. Sustain learning systematically by providing students with multiple ways to learn new things, practice their learning, question their learning processes, and
  • 2. IV. PROCEDURES draw conclusions about what they learned in relation to their life experiences and previous knowledge. Indicate the time allotment for each step. A. Reviewing previous lesson or presenting the new lesson The teacher will give the overview of the objectives and key terms for the quarter. 1. Give a big picture of Chemistry by describing it as “the study of stuff.” The teacher will recall the Big Bang nucleosynthesis and the formation of lighter elements. The teacher will recall the evidences for and describe the formation of heavier elements during star formation and evolution The teacher will introduce the following list of important terms that learners will encounter. B. Establishing a purpose for the lesson The teacher will briefly define cosmology as the study of how the universe began, how it continues to exist, and how it will end. (Offer examples of cosmologies from different religions and cultures based on their beliefs) Guide Question? 1. Do you think there is proof that any of these stories or cosmologies are true? The students will try to refresh your mind by supplying the number of protons and neutrons of each element. The Cosmic Connection The teacher will use the Think, Pair, Share protocol and ask learners to reflect and share their thoughts on the selection. Stellar Word Puzzle! The learners will encircle and write down the words which are related to star and element formation.
  • 3. C. Presenting examples/instances of the new lesson The learners will give important clues in understanding the fundamental building blocks of the universe and how life on earth is connected to stars. In the Beginning: The Nebulae! Guide Questions? Question 1: Where do you think stars come from? The learners will share their insights. Growing Older, Growing Bigger: The Red Giant Star! Guide Questions: Why do you think red giant stars are called red giants? The students will examine the diagram from your left. It illustrates an atom’s subatomic particles namely: a. protons+ b. neutrons 0 c. electrons _ Activity I.I Making Your Own Periodic Table The learners will make their own periodic table using the hypothetical elements that are given in the clues. a. P and Pr both have one electron each. Pr has a bigger atomic size. b. Od, Ri, and E are in the same series as P, C, and I. In terms of atomic size, P is the biggest while C is the smallest. E is a metal while I is a non-metal. Od is smaller than Ri in atomic size. D. Discussing new concepts and practicing new skills # 1 The learners will explore the vast universe with the countless twinkling diamonds in the sky. 1.Stars’ Starting Point of Life: The Protostar! Guide Questions: 1. What is the core of it all? The Death of a Star: Depletion of Energy! Guide Question: 1. Do you think stars explode when they die? The students will determine their quantity in a certain element How about isotope 13 Carbon? protons ____ atomic no.___ neutrons ___ atomic mass__ The learners will write the balanced nuclear reaction of the following elements under alpha, beta and gamma decay. E. Developing mastery/ Finding practical applications of concepts and skills in daily living / Making generalizations and abstractions about the lesson Activity 1- “Forget Me Not” The learners will identify the following and tell something about each of them. Activity 1- “Star in the Making The learners will demonstrate what they have learned on the formation of stars by doing any of the suggested star projects. Comic Story- create a one-page comic star’s life cycle story (cartoons or cut-outs) Activity 1-Transformation- Radiation in One! The learners will choose the letter of the symbol that represents the type of nuclear radiation Activity 1.1 The learners will write the nuclear reactions involved in the synthesis of each of the following new elements: a. Curium (Z = 96) was formed by reacting Pu – 239 with alpha particles 42He. It has a half-life of 162 days. b. Mendelevium (Z = 101) was formed by reacting En-253 with alpha particles.
  • 4. Rubrics F. Evaluating learning Activity 2 – “Twinkle, Twinkle Little Big Star, How I Wander as You Are!” The learners will relate the evolution of a star to the life cycle of a person. The students will identify the temperature of each color? Use this temperature list: 3000 °C, 4500 °C, 6000 °C, 10 000 °C, 40 000 °C Wrap up! The learners will answer the following as you look back at the things we have talked about today. 1. What is the missing link that led to the completion of the known “almost perfect” periodic table of elements? How did it lead to the discovery of synthetic elements? 2. How do scientists forge the synthesis of elements? 3. What happens during the synthesis of new elements? The students will create an inventory list of universe’s fragments into a systematic compilation that includes the new synthetic elements G. Additional activities for application or remediation V. REMARKS Prepared by Checked by JERDA U. IDIO ALIE A. BONGCAWIL Subject Teacher Assistant Principal, Senior High Department