Source-to-probe distance
The probe distance from the source mass sets the field strength in the one-mass lab.
Concept module
See how one source mass creates an inward gravitational field, how source mass and distance set the field strength, and how a probe mass turns that field into force without changing the field itself.
The simulation shows one source mass fixed at the origin, a movable probe mass in a bounded two-dimensional field region, and optional overlays for a coarse field grid, the live field arrow at the probe, the force arrow on the probe mass, equal-distance rings, and the horizontal scan line used by the graphs. Dragging the probe changes the sampled field location directly on the stage. The focused probe handle also responds to arrow keys for small position changes, and sliders provide the same controls for source mass, probe position, and probe mass. Very near the source mass, the field display uses a minimum sampling radius so the drawn arrows and response graphs stay finite and readable. This keeps the visualization bounded while preserving the correct trend that gravitational field strength grows rapidly near the source. A source mass of 2 kg at the origin produces a gravitational field of (-0.4, -0.3) at the probe (1.6 m, 1.2 m). The probe is 2 m from the source, so |g| is 0.5 in field units and points down-left. A test mass of 1 kg feels a force of 0.5 in force units toward the source. On the same radial line, doubling the distance would reduce the field strength to about one quarter.
Interactive lab
Keep the stage, graph, and immediate control feedback in one working view.
Gravitational Fields
Drag the probe to any point in the bounded field region. The inward field arrow, force arrow, scan-line graphs, compare state, and worked examples all read the same live mass-and-distance model.
Graphs
Switch graph views without breaking the live stage and time link.
Field components on the scan line
Shows how the inward field splits into horizontal and vertical components along the current horizontal scan line.
Controls
Adjust the physical parameters and watch the motion respond.
Changes the mass creating the field, so both the inward field and the force scale with M at every point.
Moves the probe left or right across both the stage and the linked scan graphs.
Moves the probe to a new horizontal scan line so the graphs sample a different field slice.
Changes only the force on the probe. It does not change the gravitational field created by the source mass.
More tools
Secondary controls, alternate presets, and less-used toggles stay nearby without crowding the main bench.
More presets
Presets
Predict -> manipulate -> observe
Keep the active prompt next to the controls so each change has an immediate visible consequence.
Try this
Equation map
Select a symbol to highlight the matching control and the graph or overlay it most directly changes.
Changes the mass creating the field, so both the inward field and the probe force scale directly with M at every point.
Equations in play
Choose an equation to sync the active symbol, control highlight, and related graph mapping.
More tools
Detailed noticing prompts, guided overlays, and challenge tasks stay available without taking over the main bench.
What to notice
Use the current prompt as a compact investigation cue. Each one points at a pattern the stage and graphs already show in the live source-mass model.
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Why it matters
Guided overlays
Focus one overlay at a time to see what it represents and what to notice in the live motion.
Overlay focus
Shows a coarse sample of the inward field direction across the stage.
What to notice
Why it matters
It makes gravitational field direction a whole-region pattern instead of something you only infer from one probe point.
Challenge mode
Tune the same one-mass field into compact targets. The checks read the live inverse-square model instead of a detached answer key.
3 of 6 checks
Suggested start
The checklist updates from the live simulation state, active graph, overlays, inspect time, and compare setup.
Source-to-probe distance
The probe distance from the source mass sets the field strength in the one-mass lab.
Field from one source mass
The gravitational field points toward the source mass and weakens with distance.
Inverse-square trend
Doubling source mass doubles the field, while doubling distance reduces it to one quarter.
Force on the probe mass
The probe mass scales the force it feels without creating a second field in this model.
Progress
Not startedMastery: NewLocal-firstStart exploring and Open Model Lab will keep this concept's progress on this browser first. Challenge mode has 2 compact tasks ready. No finished quick test, solved challenge, or completion mark is saved yet.
Try this setup
Copy the live bench state and reopen this concept with the same controls, graph, overlays, and compare context.
Stable links
Starter track
Step 1 of 50 / 5 completeNext after this: Gravitational Potential and Potential Energy.
This concept is the track start.
Short explanation
A gravitational field tells you what one kilogram of probe mass would feel at a point before you imagine any actual probe there. In this bounded lab, one source mass sits at the origin, the field always points inward toward that mass, and the size of the field follows the inverse-square distance trend.
The same source mass, probe position, and probe mass drive the stage arrows, scan graphs, compare mode, prediction prompts, worked examples, challenge checks, and quick test. That keeps field direction, field strength, and force on a test mass attached to one honest live model instead of drifting into separate rules.
Key ideas
Live gravity checks
2 kg
1.6 m
1.2 m
1. Measure the live source-to-probe distance
2. Apply the one-mass field relation
3. Resolve the current field components
Gravitational field
Inverse-square checkpoint
Prediction prompt
Check your reasoning
Common misconception
A heavier probe mass makes the gravitational field at that point stronger.
The gravitational field at a point is set by the source mass and the source-to-probe distance. The probe mass is only responding to that field.
Making the probe mass larger increases the force because F = m_test g, but the inward field arrow and the field graph stay the same until you change the source mass or the probe position.
Quick test
Reasoning
Question 1 of 4
Choose one answer to reveal feedback, then test the idea in the live system if a guided example is available.
Accessible description
The simulation shows one source mass fixed at the origin, a movable probe mass in a bounded two-dimensional field region, and optional overlays for a coarse field grid, the live field arrow at the probe, the force arrow on the probe mass, equal-distance rings, and the horizontal scan line used by the graphs.
Dragging the probe changes the sampled field location directly on the stage. The focused probe handle also responds to arrow keys for small position changes, and sliders provide the same controls for source mass, probe position, and probe mass.
Very near the source mass, the field display uses a minimum sampling radius so the drawn arrows and response graphs stay finite and readable. This keeps the visualization bounded while preserving the correct trend that gravitational field strength grows rapidly near the source.
Graph summary
The field-components graph plots the horizontal and vertical gravitational field components along the current horizontal scan line. Hovering the graph previews the same x-location on the stage.
The strength-response graph plots the field magnitude and the probe-force magnitude along that same scan line. Changing the probe mass rescales the force curve, but the field curve remains a source-mass and distance readout.
Bridge this into orbits
These suggestions come from the concept registry, so the reason label reflects either curated guidance or the fallback progression logic.
See one source mass create a negative potential well, compare how potential and potential energy change with distance, and connect the downhill slope of phi to the gravitational field on the same live model.
See why a circular orbit needs the right sideways speed, how gravity supplies the centripetal acceleration, and how source mass and radius together set orbital speed and period on one bounded live model.
Launch outward from one bounded gravity source and see how source mass, launch radius, and total specific energy decide whether the object escapes or eventually returns.