Asteroid Weight Calculator

Asteroid Weight Calculator: Estimate Celestial Body Mass :root { –primary-color: #004a99; –success-color: #28a745; –background-color: #f8f9fa; –text-color: #333; –border-color: #ddd; –shadow-color: rgba(0, 0, 0, 0.1); –card-background: #ffffff; } body { font-family: 'Segoe UI', Tahoma, Geneva, Verdana, sans-serif; background-color: var(–background-color); color: var(–text-color); line-height: 1.6; margin: 0; padding: 0; display: flex; flex-direction: column; align-items: center; padding-top: 20px; padding-bottom: 40px; } .container { width: 95%; max-width: 960px; background-color: var(–card-background); padding: 30px; border-radius: 8px; box-shadow: 0 4px 15px var(–shadow-color); margin-bottom: 30px; } h1, h2, h3 { color: var(–primary-color); text-align: center; margin-bottom: 20px; } h1 { font-size: 2.5em; margin-bottom: 30px; } h2 { font-size: 1.8em; border-bottom: 2px solid var(–primary-color); padding-bottom: 10px; margin-top: 40px; } h3 { font-size: 1.4em; margin-top: 25px; margin-bottom: 15px; 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Asteroid Weight Calculator

Estimate the mass of an asteroid based on its dimensions and estimated density.

Calculate Asteroid Weight

Sphere Ellipsoid (Prolate Spheroid) Irregular (Approximation) Select the approximate shape of the asteroid.
Enter the average diameter in kilometers. For non-spherical shapes, this is a representative value.
The longest radius of the ellipsoid.
The shortest radius of the ellipsoid.
The intermediate radius of the ellipsoid.
Typical densities range from 1000 kg/m³ (icy) to 5000 kg/m³ (rocky/metallic).

Estimated Asteroid Weight

Volume:

Mass (Metric Tons):

Mass (Earth's Moon):

Formula Used: Mass = Volume × Density. Volume calculation depends on the selected shape.

Weight vs. Density Comparison

Comparison of estimated asteroid mass for a spherical asteroid of 1 km diameter across various densities.
Key Assumptions and Typical Values
Parameter Unit Typical Range Notes
Asteroid Shape Factor Unitless 0.5 – 1.0 Approximation for volume calculation based on shape.
Density (Icy) kg/m³ 500 – 1500 Composition: Water ice, volatiles.
Density (Carbonaceous Chondrite) kg/m³ 1500 – 2500 Common type of stony asteroid.
Density (Stony) kg/m³ 2500 – 4000 Composition: Silicate rocks.
Density (Metallic) kg/m³ 4000 – 8000 Composition: Iron-nickel alloys.
Volume of 1 km Sphere km³ ~0.524 Calculated using (4/3)πr³.

Understanding Asteroid Weight and the Calculator

What is an Asteroid Weight Calculator?

An asteroid weight calculator is a specialized tool designed to estimate the mass of an asteroid. Unlike simple weight calculators for everyday objects, this tool leverages principles of geometry and physics. It requires inputs such as the asteroid's dimensions (like diameter or axes) and its estimated density. The calculator then applies mathematical formulas to derive the asteroid's volume and subsequently its mass. This is crucial for scientific research, planetary defense, and understanding the composition of celestial bodies within our solar system. The term "weight" is often used colloquially here, but the calculation fundamentally determines mass, which is an intrinsic property, independent of gravity.

Who should use it:

  • Astronomers and astrophysicists studying asteroid populations.
  • Planetary defense researchers assessing impact risks.
  • Students and educators learning about celestial mechanics and composition.
  • Science enthusiasts curious about the scale of space objects.

Common misconceptions:

  • Weight vs. Mass: Many people use "weight" interchangeably with "mass." While related, mass is the amount of matter, and weight is the force of gravity on that matter. This calculator estimates mass.
  • Uniform Density: Asteroids are not always uniform in density. Their composition can vary significantly, affecting the overall mass even for similarly sized objects.
  • Precise Shapes: Asteroids rarely have perfect geometric shapes. The calculator uses approximations (sphere, ellipsoid) which introduce some error.

Asteroid Weight Calculator Formula and Mathematical Explanation

The fundamental principle behind calculating an asteroid's mass is the relationship between mass, volume, and density: Mass = Volume × Density. The complexity lies in accurately determining the asteroid's volume based on its shape and dimensions.

Step-by-step derivation:

  1. Determine the shape: The first step is to classify the asteroid's shape. Common approximations include perfect spheres, prolate spheroids (ellipsoids), or using a general shape factor for irregular bodies.
  2. Calculate Volume:
    • Sphere: If the asteroid is approximated as a sphere, the volume (V) is calculated using the formula: V = (4/3)πr³, where 'r' is the radius (diameter/2).
    • Ellipsoid (Prolate Spheroid): For an ellipsoid with semi-axes a, b, and c, the volume is V = (4/3)πabc. If it's a prolate spheroid (like a cigar shape, often approximated for asteroids), we might use a, b, and c where 'a' is the longest axis and 'b' and 'c' are equal or near-equal shorter axes. The calculator uses three distinct axes for generality.
    • Irregular Shape: For irregular asteroids, a shape factor (often between 0.5 and 1.0) is applied to the volume of a sphere with an average diameter. V = ShapeFactor × (4/3)π(d/2)³, where 'd' is the average diameter.
  3. Convert Units: Dimensions are typically given in kilometers (km). Density is usually in kilograms per cubic meter (kg/m³). To ensure consistent units, dimensions are converted to meters (1 km = 1000 m). Volume is then calculated in cubic meters (m³).
  4. Calculate Mass: Once the volume (V) in m³ and density (ρ) in kg/m³ are known, the mass (M) in kilograms (kg) is calculated: M = V × ρ.
  5. Convert to Desired Units: The mass in kilograms is often converted to more manageable units like metric tons (1 metric ton = 1000 kg) or compared to the mass of celestial bodies like Earth's Moon.

Variable Explanations:

  • Shape: The geometric form used for volume calculation (Sphere, Ellipsoid, Irregular).
  • Diameter (d): The representative distance across the asteroid, typically in kilometers (km).
  • Semi-axes (a, b, c): The lengths of the principal axes (radii) of an ellipsoid, in kilometers (km).
  • Density (ρ): The mass per unit volume of the asteroid's material, in kilograms per cubic meter (kg/m³).
  • Radius (r): Half of the diameter, used for spherical volume calculation (r = d/2).
  • Shape Factor: A multiplier (0 to 1) used to approximate the volume of irregular shapes relative to a sphere.
  • Volume (V): The space occupied by the asteroid, calculated based on shape and dimensions, typically in cubic meters (m³).
  • Mass (M): The amount of matter in the asteroid, calculated as Volume × Density, usually expressed in kilograms (kg), metric tons, or relative units.

Variables Table:

Variables Used in Asteroid Mass Calculation
Variable Meaning Unit Typical Range
Shape Geometric approximation Categorical Sphere, Ellipsoid, Irregular
d (Diameter) Representative diameter km 0.001 – 100,000+
a, b, c (Semi-axes) Radii along principal axes km 0.001 – 100,000+
ρ (Density) Mass per unit volume kg/m³ 100 – 8000
r (Radius) Half of diameter km 0.0005 – 50,000+
Shape Factor Volume adjustment for irregular shapes Unitless 0.5 – 1.0
V (Volume) Space occupied Highly variable
M (Mass) Amount of matter kg, Metric Tons Highly variable

Practical Examples (Real-World Use Cases)

Let's explore some scenarios using the asteroid weight calculator:

Example 1: The Near-Earth Asteroid (NEA) Bennu

Bennu, the target of NASA's OSIRIS-REx mission, is an irregularly shaped asteroid. Its dimensions are roughly 0.5 km in diameter. Its estimated density is around 1300 kg/m³ (suggesting a porous, rubble-pile structure).

  • Inputs:
  • Shape: Irregular (using a shape factor of ~0.7 for approximation)
  • Average Diameter: 0.5 km
  • Density: 1300 kg/m³

Calculation Steps:

  1. Convert diameter to meters: 0.5 km * 1000 m/km = 500 m.
  2. Calculate radius: 500 m / 2 = 250 m.
  3. Approximate volume of a sphere with this radius: V_sphere = (4/3) * π * (250 m)³ ≈ 65,449,847 m³.
  4. Apply shape factor: V_actual ≈ 0.7 * 65,449,847 m³ ≈ 45,814,893 m³.
  5. Calculate mass: Mass = 45,814,893 m³ * 1300 kg/m³ ≈ 59,559,361,000 kg.
  6. Convert to metric tons: 59,559,361,000 kg / 1000 kg/ton ≈ 59,559 metric tons.

Result Interpretation: Bennu has an estimated mass of roughly 60,000 metric tons. This relatively low mass for its size indicates a porous, loosely aggregated structure, consistent with observations.

Example 2: A Hypothetical Large Metallic Asteroid

Imagine a large, dense asteroid detected in the asteroid belt, estimated to be roughly spherical with a diameter of 10 km. Its composition suggests a high metallic content, giving it a density of 6000 kg/m³.

  • Inputs:
  • Shape: Sphere
  • Diameter: 10 km
  • Density: 6000 kg/m³

Calculation Steps:

  1. Convert diameter to meters: 10 km * 1000 m/km = 10,000 m.
  2. Calculate radius: 10,000 m / 2 = 5,000 m.
  3. Calculate volume of the sphere: V = (4/3) * π * (5,000 m)³ ≈ 523,598,776,000 m³.
  4. Calculate mass: Mass = 523,598,776,000 m³ * 6000 kg/m³ ≈ 3,141,592,656,000,000 kg.
  5. Convert to metric tons: 3,141,592,656,000,000 kg / 1000 kg/ton ≈ 3,141,592,656 metric tons.
  6. Convert to Earth's Moon mass (approx. 7.342 × 10²² kg or 7.342 × 10¹⁹ metric tons): (3.141 × 10¹² tons) / (7.342 × 10¹⁶ tons) ≈ 4.28 × 10⁻⁵ Moon masses.

Result Interpretation: This hypothetical metallic asteroid would be incredibly massive, weighing over 3 trillion metric tons. While still a tiny fraction of Earth's mass (approx. 6 × 10²¹ kg), it represents a significant object in the solar system, potentially valuable for resource extraction if accessible.

How to Use This Asteroid Weight Calculator

Using the asteroid weight calculator is straightforward. Follow these steps to get your estimated asteroid mass:

  1. Select Shape: Choose the most appropriate shape category (Sphere, Ellipsoid, or Irregular) that best describes the asteroid you are analyzing. If unsure, 'Irregular' with an average diameter is often a reasonable starting point.
  2. Input Dimensions:
    • For 'Sphere', enter the Average Diameter in kilometers.
    • For 'Ellipsoid', enter the lengths of the three semi-axes (longest, intermediate, shortest) in kilometers.
    • For 'Irregular', enter the Average Diameter in kilometers. The calculator will use a default shape factor, which can be adjusted if you have more specific information.
  3. Enter Density: Input the estimated Density of the asteroid's material in kilograms per cubic meter (kg/m³). Use typical ranges (e.g., 1000-2000 kg/m³ for icy, 2000-4000 kg/m³ for rocky, 4000-8000 kg/m³ for metallic) based on spectral analysis or composition models.
  4. Calculate: Click the "Calculate Weight" button.

Reading the Results:

  • Main Result (Mass): This is the primary output, showing the estimated mass in metric tons.
  • Volume: Displays the calculated volume in cubic meters (m³).
  • Mass (Metric Tons): The primary result, easily comparable to terrestrial scales.
  • Mass (Earth's Moon): Provides context by comparing the asteroid's mass to that of Earth's Moon.
  • Chart: Visualizes how mass changes with density for a standard 1 km spherical asteroid.
  • Table: Summarizes key assumptions and typical values for density and shape factors.

Decision-Making Guidance: The results help in classifying asteroids by size and composition. A high density suggests a metallic or rocky composition, potentially valuable for resources. A low density, especially for larger objects, might indicate a rubble-pile structure, which could influence its structural integrity and potential fragmentation.

Key Factors That Affect Asteroid Weight Results

Several factors influence the accuracy of the calculated asteroid mass. Understanding these is key to interpreting the results:

  1. Shape Approximation: Asteroids are rarely perfect spheres or ellipsoids. Their irregular shapes mean that volume calculations are always approximations. Using an average diameter or shape factor introduces uncertainty. The difference between a sphere and a more complex shape can significantly alter the calculated volume and thus mass.
  2. Density Estimation: Density is perhaps the most critical and uncertain input. It depends heavily on the asteroid's composition (rock, metal, ice, volatiles) and its internal structure (solid, porous, rubble pile). Spectral analysis can provide clues, but precise density determination is challenging. A small error in density leads to a proportional error in mass.
  3. Dimensional Accuracy: Measuring the exact size and shape of distant asteroids is difficult. Radar observations, telescopic imaging, and spacecraft missions provide data, but uncertainties remain, especially for smaller or more distant objects. Errors in diameter or semi-axis measurements directly impact the volume calculation.
  4. Internal Structure: A solid, dense asteroid will have a different mass than a similarly sized asteroid composed of loosely packed rubble with significant void space. This internal structure is directly linked to density but is hard to determine remotely.
  5. Compositional Variations: Even within a single asteroid, composition might not be uniform. Different layers or inclusions could have varying densities, making a single average density value an oversimplification.
  6. Gravitational Effects & Tidal Forces: While not directly used in the basic mass calculation, the asteroid's own gravity and how it interacts with larger bodies can influence its shape and internal structure over long timescales, indirectly affecting density and mass estimates.
  7. Surface Features: Craters, fissures, and surface boulders can affect the perceived shape and overall volume, though their contribution to mass is usually minor compared to the bulk density and dimensions.

Frequently Asked Questions (FAQ)

Q1: Is "weight" the same as "mass" for asteroids?

Technically, no. This calculator estimates mass, which is the amount of matter. Weight is the force of gravity acting on that mass. However, in common usage and for comparative purposes, "weight" is often used when "mass" is meant, especially when comparing objects.

Q2: How accurate are these asteroid weight calculations?

The accuracy depends heavily on the quality of the input data (dimensions and density). For well-characterized asteroids like Bennu, estimates are reasonably good. For distant or poorly observed asteroids, the results are rough approximations.

Q3: What is a typical density for an asteroid?

Densities vary widely. Icy asteroids might be around 1000-2000 kg/m³, stony ones 2000-4000 kg/m³, and metallic ones 4000-8000 kg/m³. Many asteroids, especially smaller ones, are porous rubble piles with densities significantly lower than solid rock.

Q4: Can I use this calculator for meteorites found on Earth?

Yes, if you know the meteorite's dimensions and can estimate its density (often based on composition – stony, iron, stony-iron), you can use the calculator to find its mass. Meteorites are essentially asteroid fragments.

Q5: What does the "Earth's Moon" comparison mean?

It provides a familiar reference point. The Moon has a mass of about 7.342 × 10¹⁹ metric tons. Comparing an asteroid's mass to this helps visualize its scale relative to a large, known celestial body.

Q6: Why is the shape important?

Shape directly determines the volume calculation. A sphere is the most volume-efficient shape for a given characteristic dimension. Irregular shapes, especially those with significant concavities or protrusions, will have less volume than a sphere of the same average diameter, leading to lower mass estimates.

Q7: What if I don't know the density?

Use the typical ranges provided. If spectral analysis suggests a certain composition (e.g., C-type, S-type, M-type), you can infer a likely density range. Consult astronomical databases or research papers for known asteroid densities.

Q8: How does this relate to asteroid mining potential?

Mass and density are fundamental parameters for assessing asteroid mining potential. High-density metallic asteroids (M-type) are prime targets for valuable metals like iron, nickel, and platinum-group elements. Understanding the mass helps estimate the potential yield of resources.

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// Default diameter input ellipsoidInputs.style.display = 'none'; ellipsoidInputsB.style.display = 'none'; ellipsoidInputsC.style.display = 'none'; // Show relevant inputs if (selectedShape === 'sphere') { document.getElementById('dimension-inputs').querySelector('label').textContent = 'Diameter (km)'; document.getElementById('diameter').setAttribute('placeholder', 'e.g., 1'); } else if (selectedShape === 'ellipsoid') { document.getElementById('dimension-inputs').style.display = 'none'; // Hide diameter input ellipsoidInputs.style.display = 'block'; ellipsoidInputsB.style.display = 'block'; ellipsoidInputsC.style.display = 'block'; } else if (selectedShape === 'irregular') { document.getElementById('dimension-inputs').querySelector('label').textContent = 'Average Diameter (km)'; document.getElementById('diameter').setAttribute('placeholder', 'e.g., 0.5'); } // Ensure calculations are triggered after shape change if values are present calculateWeight(); } function validateInput(inputElement, minValue, maxValue) { var errorElement = document.getElementById(inputElement.id + 'Error'); var value = parseFloat(inputElement.value); if (isNaN(value)) { errorElement.textContent = 'Please enter a valid number.'; errorElement.classList.add('visible'); inputElement.style.borderColor = '#dc3545'; return false; } else if (value maxValue) { errorElement.textContent = 'Value cannot exceed ' + maxValue + '.'; errorElement.classList.add('visible'); inputElement.style.borderColor = '#dc3545'; return false; } else { errorElement.textContent = "; errorElement.classList.remove('visible'); inputElement.style.borderColor = '#ced4da'; // Default border color return true; } } function calculateVolume() { var shape = shapeSelect.value; var diameter = parseFloat(document.getElementById('diameter').value); var semiMajorAxis = parseFloat(document.getElementById('semiMajorAxis').value); var semiMinorAxis = parseFloat(document.getElementById('semiMinorAxis').value); var semiIntermediateAxis = parseFloat(document.getElementById('semiIntermediateAxis').value); var volume = 0; var radius = 0; var shapeFactor = 1; // Default for sphere if (shape === 'sphere') { radius = diameter / 2.0; volume = (4 / 3) * Math.PI * Math.pow(radius * 1000, 3); // Convert km to m for volume calculation } else if (shape === 'ellipsoid') { volume = (4 / 3) * Math.PI * (semiMajorAxis * 1000) * (semiMinorAxis * 1000) * (semiIntermediateAxis * 1000); // Convert km to m } else if (shape === 'irregular') { radius = diameter / 2.0; shapeFactor = 0.7; // Approximate shape factor for irregular bodies volume = shapeFactor * (4 / 3) * Math.PI * Math.pow(radius * 1000, 3); // Convert km to m } return volume; // Volume in m³ } function calculateWeight() { var diameterInput = document.getElementById('diameter'); var semiMajorAxisInput = document.getElementById('semiMajorAxis'); var semiMinorAxisInput = document.getElementById('semiMinorAxis'); var semiIntermediateAxisInput = document.getElementById('semiIntermediateAxis'); var densityInput = document.getElementById('density'); var isValid = true; if (shapeSelect.value === 'sphere' || shapeSelect.value === 'irregular') { isValid = validateInput(diameterInput, 0.001, 100000) && isValid; } if (shapeSelect.value === 'ellipsoid') { isValid = validateInput(semiMajorAxisInput, 0.001, 100000) && isValid; isValid = validateInput(semiMinorAxisInput, 0.001, 100000) && isValid; isValid = validateInput(semiIntermediateAxisInput, 0.001, 100000) && isValid; } isValid = validateInput(densityInput, 100, 10000) && isValid; if (!isValid) { resultsContainer.style.display = 'none'; return; } var density = parseFloat(densityInput.value); // kg/m³ var volume = calculateVolume(); // m³ var massKg = volume * density; // kg var massTons = massKg / 1000; // Metric tons // Moon mass in metric tons (approx) var moonMassTons = 7.342e16; var massMoonFraction = massTons / moonMassTons; mainResultSpan.textContent = massTons.toLocaleString(undefined, { maximumFractionDigits: 2 }) + ' tons'; volumeResultSpan.textContent = volume.toLocaleString(undefined, { maximumFractionDigits: 2 }) + ' m³'; massResultTonsSpan.textContent = massTons.toLocaleString(undefined, { maximumFractionDigits: 2 }); massResultMoonSpan.textContent = massMoonFraction.toLocaleString(undefined, { minimumFractionDigits: 6, maximumFractionDigits: 6 }) + ' (Moon)'; resultsContainer.style.display = 'block'; updateChart(massTons); } function copyResults() { var mainResult = mainResultSpan.textContent; var volumeResult = volumeResultSpan.textContent; var massTonsResult = massResultTonsSpan.textContent; var massMoonResult = massResultMoonSpan.textContent; var assumptions = "Assumptions:\n"; assumptions += "Shape: " + document.getElementById('asteroidShape').value + "\n"; if (document.getElementById('asteroidShape').value === 'sphere' || document.getElementById('asteroidShape').value === 'irregular') { assumptions += "Diameter: " + document.getElementById('diameter').value + " km\n"; } else { assumptions += "Semi-axes: " + document.getElementById('semiMajorAxis').value + " km, " + document.getElementById('semiMinorAxis').value + " km, " + document.getElementById('semiIntermediateAxis').value + " km\n"; } assumptions += "Density: " + document.getElementById('density').value + " kg/m³\n"; var textToCopy = "— Asteroid Weight Calculation Results —\n\n"; textToCopy += "Estimated Mass: " + mainResult + "\n"; textToCopy += "Volume: " + volumeResult + "\n"; textToCopy += "Mass (Metric Tons): " + massTonsResult + "\n"; textToCopy += "Mass (Earth's Moon): " + massMoonResult + "\n\n"; textToCopy += assumptions; navigator.clipboard.writeText(textToCopy).then(function() { alert('Results copied to clipboard!'); }).catch(function(err) { console.error('Failed to copy results: ', err); alert('Failed to copy results. Please copy manually.'); }); } function resetCalculator() { document.getElementById('asteroidShape').value = defaultValues.shape; document.getElementById('diameter').value = defaultValues.diameter; document.getElementById('semiMajorAxis').value = defaultValues.semiMajorAxis; document.getElementById('semiMinorAxis').value = defaultValues.semiMinorAxis; document.getElementById('semiIntermediateAxis').value = defaultValues.semiIntermediateAxis; document.getElementById('density').value = defaultValues.density; // Reset error messages and borders var inputs = document.querySelectorAll('.loan-calc-container input, .loan-calc-container select'); inputs.forEach(function(input) { var errorElement = document.getElementById(input.id + 'Error'); if (errorElement) { errorElement.textContent = "; errorElement.classList.remove('visible'); } input.style.borderColor = '#ced4da'; }); updateShapeInfo(); // Update visibility of ellipsoid inputs calculateWeight(); // Recalculate with default values } function updateChart(currentMassTons) { if (chart) { chart.destroy(); } var densities = [500, 1000, 1500, 2000, 2500, 3000, 3500, 4000, 5000, 6000, 7000, 8000]; // kg/m³ var masses = []; var baseDiameterKm = 1; // For comparison chart var baseRadiusM = (baseDiameterKm / 2.0) * 1000; // meters var baseVolume = (4 / 3) * Math.PI * Math.pow(baseRadiusM, 3); // m³ densities.forEach(function(density) { var mass = baseVolume * density / 1000; // tons masses.push(mass); }); // Find the index of the current mass to highlight it var currentMassIndex = masses.findIndex(function(mass) { // Compare with a small tolerance due to floating point arithmetic return Math.abs(mass – currentMassTons) < (currentMassTons * 0.01); }); chart = new Chart(chartContext, { type: 'line', data: { labels: densities.map(function(d) { return d + ' kg/m³'; }), datasets: [{ label: 'Mass (Metric Tons) for 1km Sphere', data: masses, borderColor: 'rgb(0, 74, 153)', // Primary color backgroundColor: 'rgba(0, 74, 153, 0.2)', tension: 0.1, fill: false, pointRadius: 5, pointBackgroundColor: function(context) { if (context.dataIndex === currentMassIndex) return 'rgb(40, 167, 69)'; // Success color for current return 'rgb(0, 74, 153)'; }, pointBorderColor: function(context) { if (context.dataIndex === currentMassIndex) return 'rgb(40, 167, 69)'; return 'rgb(0, 74, 153)'; }, pointHoverRadius: 7, pointHoverBackgroundColor: function(context) { if (context.dataIndex === currentMassIndex) return 'rgb(40, 167, 69)'; return '#003366'; }, pointHoverBorderColor: function(context) { if (context.dataIndex === currentMassIndex) return 'rgb(40, 167, 69)'; return '#003366'; } }] }, options: { responsive: true, maintainAspectRatio: false, scales: { y: { beginAtZero: true, title: { display: true, text: 'Mass (Metric Tons)' } }, x: { title: { display: true, text: 'Density' } } }, plugins: { tooltip: { callbacks: { label: function(context) { var label = context.dataset.label || ''; if (label) { label += ': '; } if (context.parsed.y !== null) { label += context.parsed.y.toLocaleString(undefined, { maximumFractionDigits: 2 }) + ' tons'; } return label; } } }, legend: { display: true, position: 'top' } } } }); } // Initial setup document.addEventListener('DOMContentLoaded', function() { updateShapeInfo(); // Set initial visibility based on default shape calculateWeight(); // Perform initial calculation // Initialize chart with default data updateChart(defaultValues.density * calculateVolume() / 1000); // Calculate initial mass for chart update }); // Simple Chart.js integration (assuming Chart.js library is available or included) // For a pure HTML/JS solution without external libraries, SVG or Canvas drawing would be needed. // This example uses Chart.js for demonstration simplicity. // If Chart.js is not allowed, replace this section with native Canvas or SVG drawing. // Placeholder for Chart.js library if not included externally // In a real scenario, you'd include Chart.js via CDN or local file: // // — START: Pure JavaScript Canvas Drawing for Chart — // This replaces the Chart.js dependency for a truly self-contained solution. var canvas = document.getElementById('weightChart'); var ctx = canvas.getContext('2d'); canvas.width = 700; // Set desired canvas width canvas.height = 350; // Set desired canvas height function drawChart(chartData) { ctx.clearRect(0, 0, canvas.width, canvas.height); // Clear previous drawing var densities = chartData.labels.map(function(label) { return parseFloat(label.split(' ')[0]); }); var masses = chartData.datasets[0].data; var primaryColor = 'rgb(0, 74, 153)'; var successColor = 'rgb(40, 167, 69)'; var textColor = '#333'; var borderColor = '#ddd'; var padding = 40; var chartAreaWidth = canvas.width – 2 * padding; var chartAreaHeight = canvas.height – 2 * padding; // Find max values for scaling var maxY = Math.max(…masses); var maxX = densities[densities.length – 1]; // — Draw Axes — ctx.strokeStyle = borderColor; ctx.lineWidth = 1; // Y-axis ctx.beginPath(); ctx.moveTo(padding, padding); ctx.lineTo(padding, canvas.height – padding); ctx.stroke(); // X-axis ctx.beginPath(); ctx.moveTo(padding, canvas.height – padding); ctx.lineTo(canvas.width – padding, canvas.height – padding); ctx.stroke(); // — Draw Labels and Ticks — ctx.fillStyle = textColor; ctx.font = '12px Arial'; ctx.textAlign = 'center'; // Y-axis labels and ticks var numYTicks = 5; for (var i = 0; i <= numYTicks; i++) { var yPos = canvas.height – padding – (i / numYTicks) * chartAreaHeight; var yValue = Math.round((maxY / numYTicks) * i); ctx.fillText(yValue.toLocaleString(undefined, { maximumFractionDigits: 0 }), padding – 10, yPos – 5); ctx.beginPath(); ctx.moveTo(padding – 5, yPos); ctx.lineTo(padding, yPos); ctx.stroke(); } // X-axis labels and ticks ctx.textAlign = 'center'; densities.forEach(function(density, index) { var xPos = padding + (index / (densities.length – 1)) * chartAreaWidth; ctx.fillText(density + ' kg/m³', xPos, canvas.height – padding + 15); ctx.beginPath(); ctx.moveTo(xPos, canvas.height – padding); ctx.lineTo(xPos, canvas.height – padding + 5); ctx.stroke(); }); // — Draw Data Series (Line) — ctx.beginPath(); ctx.strokeStyle = primaryColor; ctx.lineWidth = 2; ctx.lineJoin = 'round'; masses.forEach(function(mass, index) { var xPos = padding + (index / (densities.length – 1)) * chartAreaWidth; var yPos = canvas.height – padding – (mass / maxY) * chartAreaHeight; if (index === 0) { ctx.moveTo(xPos, yPos); } else { ctx.lineTo(xPos, yPos); } }); ctx.stroke(); // — Draw Points and Highlight Current — var currentMassIndex = masses.findIndex(function(mass, index) { var currentDensityVal = parseFloat(document.getElementById('density').value); var currentDensityIndex = densities.findIndex(function(d) { return d === currentDensityVal; }); return index === currentDensityIndex; }); masses.forEach(function(mass, index) { var xPos = padding + (index / (densities.length – 1)) * chartAreaWidth; var yPos = canvas.height – padding – (mass / maxY) * chartAreaHeight; ctx.beginPath(); ctx.fillStyle = (index === currentMassIndex) ? successColor : primaryColor; ctx.strokeStyle = (index === currentMassIndex) ? successColor : primaryColor; ctx.lineWidth = 1; ctx.arc(xPos, yPos, 5, 0, Math.PI * 2); // Draw circle ctx.fill(); ctx.stroke(); // Outline circle }); // — Draw Title — ctx.font = 'bold 16px Arial'; ctx.textAlign = 'center'; ctx.fillStyle = primaryColor; ctx.fillText('Mass vs. Density (1km Sphere)', canvas.width / 2, padding / 2); } // Modify updateChart to use drawChart function updateChart(currentMassTons) { var densities = [500, 1000, 1500, 2000, 2500, 3000, 3500, 4000, 5000, 6000, 7000, 8000]; // kg/m³ var masses = []; var baseDiameterKm = 1; // For comparison chart var baseRadiusM = (baseDiameterKm / 2.0) * 1000; // meters var baseVolume = (4 / 3) * Math.PI * Math.pow(baseRadiusM, 3); // m³ densities.forEach(function(density) { var mass = baseVolume * density / 1000; // tons masses.push(mass); }); var chartData = { labels: densities.map(function(d) { return d + ' kg/m³'; }), datasets: [{ label: 'Mass (Metric Tons) for 1km Sphere', data: masses, // Colors are handled in drawChart }] }; drawChart(chartData); } // — END: Pure JavaScript Canvas Drawing for Chart —

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