KamCosmosBY KAM K.H. NG
Discover The animated sky

NOTES FROM THE NIGHT SKY

The story of
deep space.

Clouds become nurseries.
Stars gather. Galaxies change.
Every light belongs to a larger story.

Follow the starlight
01 / NEBULAE02 / GALAXIES03 / STAR CLUSTERS
Three scales. Connected histories.

01 / NEBULAE

The matter
between the stars.

Gas. Dust. Possibility.

Some clouds cradle stars.
Others carry the traces of stellar endings.

Explore the science ↗
FIELD STUDY / 01An artistic particle view of a dark nebula.
Dark nebulaPARTICLE STUDY

CHOOSE A CLOUD

HIDDEN BEGINNINGS

A nursery in shadow.

Dust blocks the light behind it.
Cold, dense regions can form stars.

Material
Gas + dust
Visible clue
A dark silhouette

Emission and reflection can coexist in one cloud.

FOLLOW THE MATERIAL

One beginning.
Different stellar endings.

Stellar mass shapes the path.
Ejected gas rejoins the space between stars.

START

Cold cloud

Collapse · star formation

Stars begin to shine

A SUN-LIKE STAR

  1. Red giantOuter layers expand
  2. Planetary nebulaShed gas glows
  3. White dwarfA fading stellar core

A MASSIVE STAR

  1. SupergiantRapid fuel use
  2. SupernovaA possible explosive ending
  3. Compact remnantNeutron star or black hole
Gas returns. New clouds gather.

Shed layers and supernova ejecta enrich interstellar space.

THE MATERIAL CONTINUES

Representative paths, not every possible outcome. A planetary nebula is a stellar ending; it does not form planets.

02 / GALAXIES

Islands with
many histories.

Stars. Gas. Dust. Dark matter.

Gravity holds the system together.
Cold gas fuels new generations of stars.

Explore the science ↗
FIELD STUDY / 02An artistic particle view of a spiral galaxy.
Spiral galaxyPARTICLE STUDY
STRUCTURE / SPIRAL

A disc in motion.

Gas-rich arms often host young stars.
A central bulge often contains older stars.

Shape is not an age label.Different histories can produce similar forms.

WHAT CHANGES A GALAXY?

The supply
of fresh beginnings.

Follow the cold gas.
More fuel can mean more star formation.

01

Gather

Gas flows in.
Smaller systems assemble.

02

Grow

Cold clouds collapse.
New stars light the disc.

POSSIBLE CHANGES

Gas loss or heatingLess star formation
Gravitational encountersDisturbed shapes · new orbits
A fresh gas supplyRenewed star formation
Star-formingCold gas available
QuenchingStar formation declines
QuiescentFew new stars

A quiet galaxy still contains shining stars. Encounters do not always cause quenching.

03 / STAR CLUSTERS

Born together.
Changed by company.

Stellar families, shaped by gravity.

Some loosen and disperse.
Others remain bound for billions of years.

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OPEN CLUSTERS

Room
to wander.

Structure
Loose · irregular
Typical home
Galactic discs
Long-term story
Spreading · dispersal

Many disperse. Some survive for billions of years.

GLOBULAR CLUSTERS

Gravity
in company.

Structure
Dense · roughly spherical
Typical home
Galactic haloes
Long-term story
Internal change · tidal loss

Often ancient. Many contain multiple stellar populations.

FIELD STUDY / 03An artistic particle view of an open-cluster nursery.
Open cluster · BirthPARTICLE STUDY

COMPARE THE SAME STAGE

OPEN CLUSTER / BIRTH

A shared beginning.

Cloud fragments contract.
A loose stellar nursery takes shape.

Separate histories, not successive stages of one cluster.

OPEN
  1. GatherStars form
  2. EmergeGas clears
  3. RearrangeEnergy is exchanged
  4. DisperseMembers join the Galaxy
GLOBULAR
  1. GatherA dense beginning
  2. Remain boundA stellar system endures
  3. RedistributeThe core can change
  4. Lose starsTidal streams extend

Leaving the cluster does not mean going dark.Escaping stars keep shining.

ONE SKY · CONNECTED HISTORIES

Matter returns.
The story continues.

Return to the animated sky

Visual interpretations. Shapes, colours and motion are illustrative.

LOOK A LITTLE CLOSER

Further reading.

Selected astronomy references.
A starting point for your own exploration.