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The Sun is Also a Star Analysis for Reading 2
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In the story The Sun Is Also a Star, we get to know the two main characters, Daniel and Natasha, in a special way. The author lets us see the world through their eyes by writing from each character's point of view, switching back and forth between them.
When we read Daniel's parts, we learn what's going on inside his head. We understand how he feels about his family, his dreams, and the pressure to become a doctor. Daniel's thoughts are full of humor and clever descriptions, even when he's dealing with tough stuff.
Natasha's chapters show us her way of thinking. She's facing a scary situation with her family's deportation, and she looks at things in a realistic way. Natasha doesn't believe in fate or miracles, but she still hopes for a way to stay in America.
By giving us both perspectives, the author helps us connect with Daniel and Natasha. We see that they have different backgrounds and challenges, but they're both trying to figure out who they are and what they want. Switching viewpoints keeps the story exciting and lets us imagine how the characters might come together, even though they see the world in their own unique ways.
In The Sun Is Also a Star, the author's use of alternating first-person perspectives primarily serves to:
create a sense of confusion for the reader.
allow readers to connect with and understand both characters' thoughts and experiences.
make the story more challenging to follow.
highlight the differences between Daniel and Natasha's personalities.
Based on the information provided about Daniel's chapters, it can be inferred that his narrative voice:
is consistently serious and focused on his problems.
is indistinguishable from Natasha's narrative voice
lacks depth and fails to provide insight into his character
incorporates humor and descriptive language to convey his thoughts and feelings.
In the story The Sun Is Also a Star, we get to know the two main characters, Daniel and Natasha, in a special way. The author lets us see the world through their eyes by writing from each character's point of view, switching back and forth between them.
When we read Daniel's parts, we learn what's going on inside his head. We understand how he feels about his family, his dreams, and the pressure to become a doctor. Daniel's thoughts are full of humor and clever descriptions, even when he's dealing with tough stuff.
Natasha's chapters show us her way of thinking. She's facing a scary situation with her family's deportation, and she looks at things in a realistic way. Natasha doesn't believe in fate or miracles, but she still hopes for a way to stay in America.
By giving us both perspectives, the author helps us connect with Daniel and Natasha. We see that they have different backgrounds and challenges, but they're both trying to figure out who they are and what they want. Switching viewpoints keeps the story exciting and lets us imagine how the characters might come together, even though they see the world in their own unique ways.
In The Sun Is Also a Star, the author's use of alternating first-person perspectives primarily serves to:
Based on the information provided about Daniel's chapters, it can be inferred that his narrative voice:
Analyzing Natasha's perspective, which of the following statements best describes her approach to her family's deportation situation?
The Sun is Also a Star Analysis for Reading 3The Sun is Also a Star First 20The Sun is Also a Star Reading 1 QuizTHE SOAR SYSTEM A solar system is a group of planets and other celestial bodies that revolve around a star. A solar nebula- a vast cloud of gas and dust, mostly hydrogen and helium. How the Solar System Form • COLLAPSE AND SPINNING DISK FORMATION - Gravity pulls material inward. The cloud flattens into a spinning disk due to conservation of angular momentum. • PROTOSTAR FORMATION- (BIRTH OF THE SUN). Material collects at the center, and begun to heat up. When it reaches to 10 million KELVIN, nuclear fusion begins. thus, SUN is born. • PLANETESIMALS AND PROTOPLANETS. Dust and gas in the disk stick together via static and gravitational forces. These form planetesimals, which grow into protoplanets collision and accretion. • PLANET FORMATION. Inner disk: too hot for gas rocky planets form Mercury, Venus, Earth, Mars. • PLANET FORMATION. Outer disk: gas and ice giants. Jupiter, Saturn, Uranus, Neptune • LEFTOVER DEBRIS. Remaining materials forms moon, asteroids, comets and dwarf planets. DIFFERENT HYPOTHESIS IN THE FORMATION OF SOLAR SYSTEM. 1. NEBULAR HYPOTHESIS- The Solar system formed from a rotating cloud of Gas and Dust (solar nebula). As it rotates conservation of angular momentum caused the cloud to flatten into a disk. the Sun formed at the center (DISK) while planets formed from the surrounding materials through acceleration. thus, it explains the coplanar and nearly circular orbit of the planets all planets orbits around the sun on the same flat, disk shaped plane. Proposed by Immanuel Kant in 1755 and Modified by Pierre Simon Laplace in 1756. PROTOPLANET HYPOTHESIS. The Solar system formed from a rotating cloud of Gas and Dust (solar nebula). As it rotates conservation of angular momentum caused the cloud to flatten into a disk. 2. Protoplanet hypothesis. Builds on the nebular model but focuses more on the role of planetesimals which then form into full planets. PROCESS: - Small solid particles stick together through collisions. As collisions takes place, it grows into kilometer-sized planetesimals. Gravitational interactions lead to the formation of planets. Lead to formation of steroids belts and varying planet sizes 3. Encounter hypothesis. States that the sun encountered a rogue star. The encounter led to the removal of hot gas from both stars due to their gravitational interaction. The hot gas then accumulated and formed the planets. The materials from the less dense rogue star formed the other planets, while that from the sun formed the inner planets. 4. TIDAL HYPOTHESIS. (also called the Tidal Theory) is an early scientific idea about how the solar system might have formed. Proposed by James Jeans and Harold Jeffreys. A massive star passed very close to the early Sun. The hot gas then accumulated and formed the planets. The materials from the less dense rogue star formed the other planets, while that from the sun formed the inner planets. Streams of hot gas were drawn out from the Sun in elongated shape. These streams eventually condensed and cooled, forming planets, moons, and other bodies in the solar system. 5. Not accepted theory. Later studies showed the streams of hot gas would disperse too quickly into space instead of condensing into planets. The theory also couldn’t explain the specific orbital patterns and compositions we see today. Modern science favors the Nebular Hypothesis, which explains solar system formation through the collapse of a rotating gas cloud. Earth as the only habitable planet 1. Right Distance from the Sun (The Goldilocks Zone). Not too hot, not too cold — just right for liquid water to exist. 2. Atmosphere with Oxygen. Earth has a mix of gases, especially oxygen, which most living things need to survive. 3. Liquid Water. Earth has oceans, rivers, and rain — water is essential for all life. 4. Magnetic Field. Earth’s magnetic field protects us from harmful solar radiation. 5. Stable Climate. The atmosphere and natural cycles keep temperatures and weather mostly stable over time. 6. Rich Resources. Earth has soil for growing food, minerals, and energy sources that support life and technology. Solar explorations 1. AUGUST 6, 2014. First space craft to orbit a comet (ROSETTA PROBE). Captures the comet photograph. -Comets have coma and tail as it approaches to the sun. 2. JULY 14, 2015. NASA’s New Horizons spacecraft made history by becoming the first spacecraft to fly by Pluto, giving us our first close-up look at the dwarf planet. First time visiting Pluto. Before this, Pluto was just a blurry dot in telescope images. Revealed a surprising world New Horizons showed mountains of ice, smooth plains, and a heart-shaped region called Tombaugh Regio. Changed what we knew. Scientists thought Pluto would be dull and frozen — instead, it turned out to be geologically active and incredibly complex. 3. SEPTEMBER 8, 2016. NASA launched OSIRIS-REx, the first U.S. mission to collect a sample from an asteroid and return it to Earth. Changed what we knew. Scientists thought Pluto would be dull and frozen — instead, it turned out to be geologically active and incredibly complex. OSIRIS-REx stands for: Origins, Spectral Interpretation, Resource Identification, Security–Regolith Explorer It was sent to study the asteroid Bennu, a near-Earth asteroid about 500 meters wide. Mission Goals: Collect a sample of surface material from Bennu Study the asteroid’s omposition, structure, and history. Mission Goals: Help scientists understand the origins of the solar system. Learn more about asteroids that could impact Earth. 4. August 12, 2018: Launch of NASA’s Parker Solar Probe, the first spacecraft to "touch" the Sun by flying through its outer atmosphere, called the corona. Mission Goal: To study the Sun up close and help scientists understand: How the solar wind (a stream of charged particles) is formed. Why the Sun’s corona is hotter than its surface. What causes solar storms that can affect Earth’s satellites and power grids. 5. November 26, 2018: NASA’s Insight Lander Touches Down on Mars. Its mission was focused on studying the interior of the Red Planet (crust, mantle, and core of the planet). Why the Sun’s corona is hotter than its surface. What causes solar storms that can affect Earth’s satellites and power grids 6. November 26, 2018: NASA’s Insight Lander Touches Down on Mars. Its mission was focused on studying the interior of the Red Planet (crust, mantle, and core of the planet) 7. JULY 30, 2020 PERSEVERANCE PROBE. Perseverance rover as part of the Mars 2020 mission aboard an Atlas V-541 rocket This marked a major step in Mars exploration. 8. DECEMBER 25, 2021-JAMES WEBB SPACE TELESCOPE. Investigate exoplanets’ atmospheres for signs of habitability. Observe the first galaxies formed after the Big Bang. Study the formation of stars and planetary systems. Look deeper into the infrared universe than ever before. RESULTS OF EXPLORATION • Evidence of Ancient Life-friendly Environment. • Sedimentary rocks formed in water-rich environments. • Signs of clay and carbonate minerals, which can preserve biosignatures (traces of past life). • Evidence of Ancient Life-friendly Environment. • Sedimentary rocks formed in water-rich environments. • Signs of clay and carbonate minerals, which can preserve biosignatures (traces of past life). • Evidence of Ancient Life-friendly Environment. • Sedimentary rocks formed in water-rich environments. • Signs of clay and carbonate minerals, which can preserve biosignatures (traces of past life).During daytime, the sky is bright and clear because the sun shines bright. We can see clouds, the sun and sometimes there is a rainbow. The sun is the nearest and brightest star on earth, the reason why we don’t see stars during daytime because the sun overpowers the weak lights of the stars. Do you know that the sun changes its position at different time of the day? Yes, early in the morning we can see the sun rising at the East. At this time of the day our surroundings is bright but not very hot, this is the reason why many children especially new born are placed under the sun because the light coming from the sun is good for them. At noontime the sun is overhead. It is very hot at this time of the day. This is the reason why it is not advisable for us to go outside. In the afternoon, we can see the sun setting at the West part of the sky. It is said that this the best time for the children to play outside because the sky s less bright and the temperature is cooler. SCIENCE 2 – MODULE 10 SEIBO COLLEGE 5 It is during daytime we do our chores, like cleaning the house, washing clothes, going to school or office and play. What do you think the reason why we do all these things during daytime? Now, close your eyes then imagine it is nighttime already. What can you see in the sky? Open your eyes then observe the picture below. Can you see these? Very good! You can see the moon and the stars. Sometimes you can see shooting stars or falling stars. At nighttime, we can not see the sun because it is already dark, we can only see the moon and the stars twinkling in the sky. Since there is no sun at night, the temperature is cooler. This is also the best time for us to rest and sleep. Do you know that the moon doesn’t have its own light? Yes, the moon only reflects the light from the sun. Do you now understand the difference of daytime from nighttime? Very good! But the question is how and why do we experience day and night? We experience day and night because the earth is moving around its axis. This movement is called rotation. SCIENCE 2 – MODULE 10 SEIBO COLLEGE 6 When the earth continuously rotates on its axis, part of it faces the sun and the other part is dark. The part of the earth that faces the sun experience daytime and the other part that is dark experience nighttime.Do you know where do the things around us get the energy they are using? How about you? Where do you get the energy you need to do your daily activities? Do you remember what we have discussed in Unit 4? Very good! OBJECTIVES: - Names the sources of energy. - Classifies the different sources of energy. SCIENCE 2 – MODULE 6 SEIBO COLLEGE 4 Energy allows us and all the things around us to move, work and become useful. Different things use different sources of energy. Let us find out what are these sources. Let us begin with the major source of energy, the sun. Sun The sun is most important and the main source of energy on earth. It makes the day hot, dry and bright. It can also help in… a. drying our clothes b. growing of plants Do you know that the sun is a star? Yes, the reason why we could see it during day time is that it is the nearest star to our planet. Electricity Electricity allows electrical appliance work. SCIENCE 2 – MODULE 6 SEIBO COLLEGE 5 Fuel Fuel makes different kinds of vehicles move. We use different kinds of vehicles to transport us from one place to another place. Food Like what we have discussed in unit 4, we get the energy we need to do our daily activities from the food we eat.Here's how scientists figured out the age of the universe It took some cosmic detective work. by Passant Rabie Oct. 20, 2021 You never ask a cosmic being its age. But if that cosmic being encompasses all of space, time, and matter, you could get a little curious. Scientists have long been curious about the age of the universe and how much time has elapsed since the Big Bang. Today, scientists estimated the age of the universe to be approximately 13.8 billion years old. But how did scientists estimate how old the universe is, and are they sure of that number? It all comes down to ancient stars and the ever-expanding cosmos. How do astronomers calculate the age of the universe? To estimate the age of the universe, scientists rely on two main methods. Calculating the expansion rate of the universe Determining the ages of the oldest stars The Hubble Constant: Since its conception, the universe has been expanding at an accelerating rate. The universe’s expansion rate is known as the Hubble Constant, which is estimated at 46,200 mph per million light-years. The Hubble Constant was first calculated in the 1920s by American astronomer Edwin Hubble after discovering that several galaxies were moving away from Earth. Scientists looked to distant galaxies to measure how fast the universe was expanding. Hubble also noted that the further a galaxy was, the faster it was moving away. Based on Hubble’s observations, the astronomer came up with Hubble’s law which showed a correlation between how far an object is and the speed at which it’s receding. Using Hubble law, scientists were able to estimate the expansion rate of the universe. Scientists were then able to use the Hubble Constant to estimate the age of the universe by working backward, all the way back to the Big Bang. This extrapolation depends on the current density and composition of the universe, which shows the history of its expansion. In 2012 NASA’s Wilkinson Microwave Anisotropy Probe used that data to estimate the universe's age to be 13.772 billion years old, give or take 59 million years. A year later, The European Space Agency’s Planck spacecraft estimated the universe's age to be 13.82 billion years. Ancestral stars: Another way to determine the age of the universe is to look to the oldest stars. The universe can’t be younger than its oldest stars. Therefore, to narrow down the age of the universe, scientists measure the ages of the very first stars that formed in the cosmos. The lifecycle of a star depends on its mass, with high mass stars burning fuel at a faster rate and therefore dying out faster while low mass stars can live up to 20 billion years. Globular clusters are a dense stellar collection of around a million stars which all formed roughly around the same time. These clusters can then serve as timekeepers for the universe. By determining the masses of their stars, scientists can estimate when the globular cluster formed. The oldest globular clusters contain stars that are 0.7 times less massive than the Sun, which suggests that they are between 11 to 18 billion years old. What came before the Big Bang? Scientists can trace the universe back to its explosive birth, the Big Bang. But what happened before this theoretical birth of the cosmos? The universe may have been a singularity, all compact within a form that is smaller than a subatomic particle. It’s difficult to imagine what caused this matter to exist, but one theory even suggests that our universe was born from another universe while another imagines a series of universes being born out of one another like a formation of bubbles. Meanwhile, another theory suggests that the universe goes through an endless cycle of death and rebirth, born from its own demise. How old is the universe in seconds? If the universe is indeed cyclical, then time becomes irrelevant. But just in case you’re still attached to the modern way in which we measure the progression of life, then the age of the universe comes up to about 436,117,076,900,000,000 seconds.Got you now 👍 — you don’t want a code, you want ready-made quiz content you can paste into Quizalize so a teacher/class can use it. I’ll generate a proper SSS1 quiz bank (Maths, English, Basic Science) in a clean format. You can copy this into Quizalize “Create Quiz”. 📘 SSS1 QUIZ (READY FOR QUIZALIZE) 🧠 MATHS (10 QUESTIONS) What is 9 × 8? 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