Start where you are
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https://blackhole.org/universe/start/
You do not need to know the names of constellations, own a telescope, or remember a physics formula to begin. Astronomy starts with noticing a pattern and asking what could explain it. This section helps you move from that first question to a picture, a measurement, and a reasoned explanation.
Start with something you can picture
Section titled “Start with something you can picture”Why does the Moon change shape? is a useful first stop. The visible pattern is familiar, but explaining it requires you to imagine the same Moon from two viewpoints. You can investigate it with a diagram or the linked laboratory, indoors and in daylight.
If another question interests you more, start there:
- Other worlds: How do we find planets around other stars?
- Light: What can starlight tell us?
- Extreme gravity: Black Holes: Start Here
- Life: Are we alone?
Try three ways into astronomy
Section titled “Try three ways into astronomy”- A familiar observation: predict a quarter Moon, then compare the two viewpoints.
- A surprising comparison: double a model planet’s radius and inspect two transits on the same axes. Does the lost light double too?
- Real measurements: inspect four absorption features in Vega’s observed spectrum. Separate what the telescope measured from the pattern used to interpret it.
Each is a short starting point. You do not need to finish a journey before trying one.
Choose how far to take the question
Section titled “Choose how far to take the question”The main explanation uses ordinary language and labeled diagrams. Prediction activities ask you to predict, compare, measure, or explain. Optional mathematics sections add a quantitative argument; the preparation is stated where it is needed. Opening or skipping one does not change the rest of the page.
Reading and activity times are approximate. Taking longer to draw a diagram or revise an explanation is part of the investigation.
Use a model thoughtfully
Section titled “Use a model thoughtfully”A model keeps selected features of a situation and leaves others out. A flat Moon-orbit drawing helps explain phases, but cannot predict an eclipse on a particular date. A smooth transit curve helps connect a planet’s size to a dip in starlight, but a real telescope records noise and other effects too.
At each result, ask three questions:
- What was actually observed or measured?
- What assumptions connect that measurement to the explanation?
- What else would we need to check?
Those questions are useful even when you do not use equations.
Keep your place
Section titled “Keep your place”Choose a journey for a connected sequence. Bookmark the current article or keep its tab open to return later. The site does not store your answers or maintain a student account.
Use Print activity for the article’s explanation and tasks with marked answers and educator notes omitted. Print with explanations includes the answers, optional mathematics and source details. The screen returns to your previous disclosure state afterward. Without scripting, open the sections you want before printing and check the preview.
Make your first prediction
Section titled “Make your first prediction”Imagine an astronaut standing on the Moon. Does the Sun illuminate a different amount of the whole Moon when we see a crescent from Earth?
Think it through
Approximately half the Moon is sunlit at a time. What changes through the phases is how much of that sunlit half we can see from Earth. The Moon article builds the geometry behind that answer.