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Available for Windows

Makarov Astronomy Suite

120 interactive modules in six rings connect planets, stars, galaxies and cosmology with observation and spaceflight. Follow an orbit, inspect a star’s changing behaviour, explore a black hole or take control of a machine working beyond Earth.

120 modules · Page 5 / 6

81Earth's wandering pole — Actual application image

Astronomy

Earth's wandering pole

Scrub through 25,772 years. Follow the axis around the ecliptic pole and see why the pole star changes.

82Earth's orbital climate rhythms — Actual application image

Astronomy / Earth

Earth's orbital climate rhythms

Compare eccentricity, tilt and precession with summer sunlight at a selected latitude. Move through 400,000 years.

83Sunlight nudges an asteroid — Actual application image

Astronomy

Sunlight nudges an asteroid

Reverse the spin-axis tilt to reverse the diurnal Yarkovsky drift. Change thermal inertia to move the afternoon hot spot.

84When planets migrate together — Actual application image

Astronomy

When planets migrate together

Compare slow and fast convergent migration. Watch an imposed 2:1 resonance retain the period ratio as the pair moves through the disk.

85A passing star wakes the comet cloud — Actual application image

Astronomy

A passing star wakes the comet cloud

Move a stellar flyby closer and count comet orbits whose new perihelia enter the giant-planet region. Red tracers identify those orbits.

87Reconstructing an unseen asteroid — Actual application image

Astronomy

Reconstructing an unseen asteroid

Watch a star disappear behind an asteroid. Change the observing track and combine multiple chords to infer the object's size and shape.

88Reading the light of two stars — Actual application image

Astronomy

Reading the light of two stars

Tilt a binary orbit until eclipses appear. Unequal eclipse depths reveal different surface brightnesses; their widths constrain stellar radii.

89A star's bow wave — Actual application image

Astronomy

A star's bow wave

Balance an outward stellar wind against an incoming interstellar flow. Change density or speed and watch the stand-off distance respond.

90The radioactive light of a supernova — Actual application image

Astronomy

The radioactive light of a supernova

Follow an expanding Type Ia remnant through its first hundred days. Compare nickel mass, diffusion time and apparent brightness at different distances.

91Between a planet and a star — Actual application image

Astronomy

Between a planet and a star

Increase the mass while keeping a Jupiter-sized object in view. Compare cooling brown dwarfs with objects capable of sustained hydrogen fusion.

93A sunset bent by the air — Actual application image

Astronomy

A sunset bent by the air

Lower the Sun toward the horizon. Compare its geometric and refracted positions, flattening and the effect of atmospheric turbulence.

94Unpacking starlight with a grating — Actual application image

Astronomy

Unpacking starlight with a grating

Send light through a slit and diffraction grating onto a detector. Change groove density, illuminated width and radial velocity to separate resolution from Doppler shift.

96A planet hidden in a star's wobble — Actual application image

Astronomy

A planet hidden in a star's wobble

Separate proper motion, annual parallax and the smaller reflex orbit caused by a planet. Compare the wobble with the chosen measurement noise.

98The invisible halo around a galaxy — Actual application image

Astronomy

The invisible halo around a galaxy

Build a Navarro–Frenk–White halo. Probe its enclosed mass, circular speed and light deflection at different galactic radii.

99Stretching a tiny patch of the Universe — Actual application image

Astronomy

Stretching a tiny patch of the Universe

Increase the number of e-folds. Compare exponential expansion with a shrinking comoving Hubble radius and follow a perturbation as it crosses that scale.

100How many voices could share the Galaxy? — Actual application image

Astronomy

How many voices could share the Galaxy?

Change the assumptions in the Drake equation. Explore how communicative lifetimes and uncertain biological fractions change the expected number of contemporaries.

Some modules belong to more than one Suite. Shared experiments have one description here.