What does a student learn in StateAlabama,GradeGrade 6,SubjectScience?

Students practice turning a fuzzy question into a testable one by naming what they will change, what they will measure, and what they expect to happen.

Students build diagrams, charts, or physical models to explain ideas they can't see directly, like how molecules move or how a system works. Then they test and revise those models when new evidence comes in.

Students plan and run experiments that change one thing at a time, track multiple variables, and use the results to explain what they found or solve a problem.

Students look at data from experiments, decide whether two things are truly connected or just happening at the same time, and use basic statistics to check how reliable the results are.

Students look for patterns in large sets of data and use numbers or math to back up their conclusions. Think of it as finding a trend in a table or graph and then explaining what the numbers actually mean.

Students back up their explanations with evidence from more than one source, making sure that evidence lines up with what science already knows about the topic.

Students build a science argument by connecting a claim to real evidence, then explain why that evidence supports or challenges an explanation or a solution. The reasoning has to hold up, not just sound convincing.

Students read scientific sources and judge whether the evidence and reasoning actually hold up. They look for weak logic, missing data, or claims that go further than the evidence supports.

Students move and adjust physical or digital models to show how the sun, Earth, and moon travel in predictable, repeating paths. The focus is on patterns: why we see day and night, monthly moon phases, and yearly seasons.

Students explain why Earth has days, years, and seasons by studying how Earth moves around the sun and spins on its tilted axis. Position and tilt, not distance, are what change the seasons.

Students explain why the moon appears to change shape each night, why eclipses happen, and why ocean tides rise and fall, all by tracing those patterns back to where the sun, moon, and Earth are positioned relative to each other.

Students look at how ideas about the universe have changed, from early models that placed Earth at the center to modern understanding of galaxies and deep space. The goal is to explain why scientists updated those ideas as new evidence appeared.

Gravity is the force that keeps planets circling the sun, moons orbiting planets, and satellites staying on course. Students explain, using evidence, how gravity controls the motion of natural and human-made objects across the solar system.

Students compare the sizes, distances, and orbits of planets and other objects in our solar system using real data. They also look at what each object is made of and whether it could support life.

Students look for repeating patterns in data, graphs, and charts to figure out why something in nature happens the way it does. A pattern in numbers or images can point to a cause hiding at a scale too small to see directly.

Students learn the difference between "X caused Y" and "X tends to happen alongside Y." They also practice using cause-and-effect patterns to predict what will happen next in nature or in a machine, including situations where an outcome has more than one cause.

Students learn that the same event, like a storm or a chemical reaction, looks different depending on how close or far you zoom in. They use models and simple equations to compare measurements and understand why size and speed matter in science.

Systems are made of smaller parts and connect to larger ones. Students use models like diagrams or charts to show how the parts interact, while recognizing that no model captures everything about the real system.

Atoms are never created or destroyed, just rearranged. Students trace how matter and energy move through systems, like heat driving wind or chemical reactions rearranging atoms into new substances.

Students examine how the shape and makeup of something, from a cell to a bridge, determines what it can do. Designs work when the right materials are shaped the right way for the job.

Small shifts in one part of a system can ripple into big changes somewhere else. Students examine what keeps natural and human-made systems stable, what disrupts them, and how tiny changes at the atomic level can add up over time.

Volcanoes, earthquakes, erosion, and weathering are constantly reshaping the land. Students study how these building-up and breaking-down forces work, and they use real evidence to explain why Earth's surface looks the way it does.

Rocks form through a cycle of heating, cooling, pressure, and erosion. Students build and use models to show how those forces change one type of rock into another over time.

Rocks form in three ways: from cooling lava, from layers of sediment that harden over time, or from existing rocks squeezed and heated deep underground. Students examine a rock's texture and minerals to identify which process made it.

Rocks and soil break apart, get carried away by water or wind, and settle somewhere new. Students model how weathering chips rock over time and how erosion moves those pieces to build up new landforms like deltas or sand dunes.

Students use research and evidence to explain why oil, coal, drinkable water, and useful minerals aren't spread evenly across the planet. The explanation connects each resource to the geologic process that formed or moved it over millions of years.

Tectonic plates are giant slabs of rock that slowly shift, collide, and pull apart over millions of years. Students explain, using evidence, how that movement builds mountains, opens ocean basins, and reshapes the ground beneath our feet.

Heat moves from deep inside Earth toward the surface. Students explain how that flow of internal energy shapes what happens at Earth's crust, using evidence to back up their reasoning.

Tectonic plates shift slowly beneath our feet, and where they meet, pull apart, or scrape past each other, the results can be dramatic. Students explain how those plate movements cause earthquakes, volcanoes, and the formation of mountains and ocean trenches.

Students use fossil locations, rock types, and the shapes of continents to piece together how Earth's plates have shifted over millions of years. The evidence shows where landmasses once fit together like puzzle pieces.

Students study rock layers and fossils to piece together a timeline of what happened on Earth millions of years ago, from ancient oceans to the first animals that left traces in stone.

Students explain why water evaporates, forms clouds, and falls as rain by tracing each step back to heat from the sun. The sun is the engine that keeps water moving between the ground, the air, and the sky.

Students investigate why the beach sand burns your feet while the water stays cool. They measure how quickly air, land, and water absorb and release heat from the sun.

Students build or draw a model showing why warm, less-dense air or water rises while cool, denser material sinks. That cycle of rising and sinking is convection, and it drives wind, ocean currents, and weather patterns.

Students read real weather data, like temperature trends or storm patterns, to spot what's coming and assess how severe weather could affect people and places.

Students collect and compare data about air masses, focusing on temperature, air pressure, and moisture levels. This data helps explain why weather changes from one day to the next.

Air pressure, weather fronts, and air masses work together to create storms, temperature swings, and rain. Students explain how those forces interact to produce the weather patterns we see day to day.

Students design and test plans to reduce damage from storms, floods, or other extreme weather. The focus is on what makes a solution work and how to improve it.

Students study how sunlight, wind, soil, and water work together to shape the climate of a place. They use real data from investigations, not just a textbook description, to explain why some regions are warmer, wetter, or drier than others.

Students learn why wind and ocean currents move the way they do. Uneven heating from the sun and Earth's spin push air and water into predictable patterns, from the breeze outside to major ocean flows that circle the globe.

Earth's tilt and curved surface mean sunlight hits some regions head-on and others at a steep angle. Students explain why places near the equator stay warm year-round while regions closer to the poles stay cold.

Students learn why some places on Earth are hotter, colder, wetter, or drier than others. Height above sea level, heat escaping from inside the Earth, and the way oceans hold and move warmth all shape the normal weather a region gets year after year.

Students examine how human choices, like burning fuel or clearing land, change Earth's air, water, and soil over time. They also look at how a growing world population puts more pressure on the environment.

Students identify a real environmental problem, such as water pollution or habitat loss, then sketch out a plan to reduce the damage or track how bad it has gotten.