Vol. Science · Astronomy · The push
Sunlight carries momentum. At 1 au the nominal irradiance is 1,361 W/m², the IAU 2015 Resolution B3 conversion constant, not a claim that the Sun is always that bright. It thins as 1/r². Divided by c = 299,792,458 m/s, a perfect absorber, face-on, feels 4.540 μN/m². A perfect reflector sends the light back, so the momentum change doubles: 9.080 μN/m², about 9.1 micronewtons on a square metre. On a flat sail, fraction ρ of the light is reflected and the rest is absorbed. Tilt θ is the angle of the sail normal from the outward Sun line. The force is (S A cos θ / c) · [(1−ρ) along the Sun line + 2 ρ cos θ along the normal]. Characteristic acceleration is that sail face-on at 1 au. The lightness number is the radiation acceleration divided by solar gravity, with the same resolution’s GM☉ = 1.3271244×10²⁰ m³ s⁻². Kopp & Lean 2011 measured 1360.8 ± 0.5 W/m² at the 2008 minimum. That measurement is not the number in the formula. A burn’s price is the rocket desk. The wait for the light itself is the light-time desk.
Educational calculator. Ideal flat sail. No thermal re-radiation, no wrinkles, no planet’s shadow, and no atmosphere. The Δv line holds this acceleration fixed: Δv = a × t. A real sail moves, the irradiance changes, and the orbit curves. Not a trajectory and not for mission design.
Sun at the left · outward is to the right · prograde is up
Distance from the Sun
Distance from 0.2 to 40 AU.
Area from 1 to 10,000 m².
Mass from 0.5 to 2,000 kg.
Reflectivity from 0 to 1.
Tilt from −90° to 90°.
Area and mass from a cited spacecraft, then a perfect reflector at 1 AU
Time, if this acceleration stayed constant
Time from 0 to 3,652.5 days.
Opens on 1 m² and 1 kg, a perfect reflector, face-on, at 1 AU. The arrow length is the force beside that perfect reflector at this distance. The direction is the force. Prograde is a circular orbit’s direction, so a positive tilt points toward it.
| Sail | Area | Mass | Force | Acceleration | Lightness | Δv, 1 day |
|---|---|---|---|---|---|---|
| 1 m² · 1 kg | 1 m² | 1 kg | 9.080 μN | 9.080 μm/s² | 1.531×10⁻³ | 0.784 m/s |
| IKAROS | 196 m² | 307 kg | 1.780 mN | 5.797 μm/s² | 9.775×10⁻⁴ | 0.501 m/s |
| LightSail 2 | 32 m² | 4.93 kg | 290.548 μN | 0.0589 mm/s² | 9.938×10⁻³ | 5.092 m/s |
| ACS3 | 80 m² | 16 kg | 726.369 μN | 0.0454 mm/s² | 7.656×10⁻³ | 3.922 m/s |
What the push is
Tiny, and it does not switch off. At 1 AU a perfect reflector, face-on, feels 9.080 μN/m², about 9.1 micronewtons on a square metre. On the 1 m², 1 kg reference that acceleration is 9.080 μm/s². A day of it, held constant, is 0.784 m/s. A Julian year of 365.25 days, still held constant, is 286.53 m/s. The push is tiny beside a rocket burn, and the sunlight does not switch off. Lightness 1, the same perfect reflector held face-on, would take 1.531 g/m². The reference sail is 1 kg/m².
Reflection is a second push. An absorbed photon hands the sail its momentum, E/c. Face-on, the pressure is the irradiance divided by c, 4.540 μN/m² at 1 AU. A reflected photon leaves carrying that momentum the other way, so the sail is pushed twice: once by the arrival and once by the departure. The face-on reflector is 9.080 μN/m². The slider is the fraction between those two. Thermal re-radiation of the absorbed energy is left out.
Tilt is how the orbit spirals. On a circular orbit the velocity is sideways, perpendicular to the Sun line. Face-on, the force is radial, so at that instant it does no work. Tilt the sail and a reflected photon leaves at an angle. For a perfect reflector the force follows the sail normal. Tip that normal forward, along the motion, and the sail gains orbital energy and spirals outward. Tip it backward and the sail loses energy and spirals inward. A perfect absorber has no transverse force in this model. The photons it catches were traveling radially, and absorbing them does not turn that momentum sideways.
What the mission buttons are
1 m² and 1 kg is a ruler. It is not a spacecraft. Face-on, the acceleration in micrometres per second squared equals the pressure in micronewtons per square metre. The other buttons replace the area and the mass, then set a perfect reflector, face-on, at 1 AU, so the comparison is this page’s ideal. None of those spacecraft was that reflector, and none of them is given an orbit here.
IKAROS is a side and a wet mass. The JAXA project page prints a square of side 14 m, a cross section of 20 m after deployment, and a liftoff mass of about 310 kg. Tsuda et al. print sail size 14×14 m and a wet mass of 307 kg, including fuel 20 kg and the sail 16 kg. The button is 14×14, which is 196 m², and 307 kg. The public about 310 kg is not substituted. A 20 m diagonal is the same square’s corner-to-corner length, not a second area.
LightSail 2 is 32 m² and 4.93 kg. Mansell et al. 2023, Table 2, prints mass 4.93 kg and sail area 32 m². Bruce Betts of The Planetary Society is a coauthor. The mission’s SciTech table prints the same pair. That paper’s introduction says 5 kg. The FCC orbital debris assessment prints 4.85 kg and 32 m². The button uses 4.93 kg and 32 m². The 5 kg and the 4.85 kg are not substituted. LightSail 2 flew an on/off cycle in Earth orbit. This button does not.
ACS3 is 80 m² and 16 kg, as a design table. Wilkie, Small Satellite Conference 2021, SSC21-II-10, prints a total deployed sail area of 80 m². The appendix table prints a total spacecraft mass, including the sail, of 16 kg, and each quadrant at 20 m². NASA’s mission page says about 80 square meters. The button uses 80 m² and 16 kg. The same table prints an effective characteristic acceleration of 0.045 mm/s² and an effective lightness number of 0.0077, with specular reflectance 0.74 on the aluminum face. This page’s perfect reflector computes 0.0454 mm/s² and lightness 7.656×10⁻³. Those effective figures are not copied. Wilkie also prints the order of a perfect reflector at 1 AU as 9×10⁻⁶ Pa. This page’s 9.080 μN/m² is the nominal 1,361 W/m² divided into c, twice.
Literacy · the words on the readout
Sources · the constants and the sails
Classroom picture of radiation pressure on a flat sail. The irradiance is the IAU 2015 nominal 1361 W/m², not the Kopp & Lean 1360.8. c and the astronomical unit are exact. GM☉ is the IAU 2015 nominal 1.3271244×10²⁰ m³ s⁻². A perfect reflector, face-on, at 1 AU feels 9.080 μN/m². Mission buttons are cited area and mass, then this ideal. Not a trajectory and not for mission design. Earthrise preview: NASA / Bill Anders (public domain).
Keep going
The burn
Δv = ve · ln(m0/mf). A sail spends no propellant. The rocket desk is what that propellant would have cost.
The delay
The same c, used as a clock. 1 AU is 8.317 minutes. Here c turns irradiance into a pressure.
The coast
Half an ellipse between two circles. Earth to Mars is 258.88 days. A sail does not fly that coast.
The year
The planet snaps are that desk’s fact-sheet semimajor axes in AU. P² = a³ is a clock. This page uses the distance.
Map
The neighborhood the sail is pushed through. Day and local time, still a schematic.
A classroom flat sail. Not a flight plan.
| Distance | 0.2 to 40 AU, on a logarithmic slider. 1 AU is the nominal irradiance. Mercury, Venus, Earth, Mars, and Jupiter are the fact-sheet semimajor axes. Earth is 1.00000011 AU. |
|---|---|
| Area and mass | Area from 1 to 10,000 m². Mass from 0.5 to 2,000 kg. Both sliders are logarithmic. |
| Reflectivity | 0 is a perfect absorber. 1 is a perfect reflector. The number accepts the same range. |
| Tilt | −90° to 90°. Zero is face-on. Positive tips the push toward prograde. The diagram’s Left and Right keys step it by one degree. |
| Presets | 1 m² · 1 kg, IKAROS, LightSail 2, and ACS3 set the area and the mass, then a perfect reflector, face-on, at 1 AU. They do not store a flight reflectivity. |
| Time | 0 to 3,652.5 days. The buttons are 1 day, 30 days, and 365.25 days. Δv = a × t, with the acceleration held fixed. A day is 86,400 seconds. |
| Irradiance | 1,361 W/m² over the square of the distance in AU. |
|---|---|
| Pressure and force | The force from the flat-sail formula, and that force divided by the area. |
| Acceleration | Force divided by mass, at this distance and tilt. |
| Characteristic | Face-on acceleration at 1 AU for this area, mass, and reflectivity. |
| Lightness | This acceleration divided by solar gravity at this distance. It does not change when only the distance changes. |
| Δv | Acceleration times the time you set. Labeled as a constant-acceleration simplification. |
| Buttons | Enter or Space selects. The pressed button is aria-pressed. Targets are at least 44 pixels on a side. |
|---|---|
| Phone | Below 900 pixels the long section row becomes a single Sections control. Open it for the same links. The site menu is the Menu button in the top bar. |
| This dialog | The question mark, or ?, opens it. Escape closes it. Tab stays inside until you close it. Click the dim page behind the card to close it. |