A Dream Eclipse Above a Giant Moon: How to Record Which Sky Layer Disappears First

Record the eclipse above the giant moon in a sequence of matched sketches. Keep their positions consistent, label each visible sky layer, and distinguish the first change from the first complete disappearance.

The task is to preserve a particular arrangement and its changes: an eclipse above a giant moon, with sky layers disappearing in an order. The supplied scene does not identify those layers or state which disappears first. A faithful record therefore needs a way to show the order that is available while leaving missing details unresolved.

The method below combines a fixed reference sketch, a layer inventory, and a sequence of before-and-after states. The drawing techniques come from visual-editing documentation; their application here is an editorial recording method. The sources explain layers, transparency, and frame comparison. They do not report this dream.

Establish the Eclipse–Moon Geometry Before Recording Changes

Begin with one reference sketch showing the eclipse above the giant moon. Preserve that vertical relationship throughout the sequence. Do not silently turn the giant moon into the eclipsed object: keep the two descriptions distinct unless the scene itself establishes their connection.

Record the moon’s apparent size through its relationship to the picture boundary and the eclipse. Does the moon fit inside the view, or does part of its edge extend beyond it? Is there a visible gap between its upper edge and the eclipse? Is the eclipse centered above it or offset? Answer only what is available. Where a measurement is uncertain, a phrase such as “large gap; exact distance unknown” preserves more information than an invented proportion.

Use the same picture boundary for every subsequent sketch. Trace or copy the reference geometry so that a shrinking gap, moving edge, or changing diameter appears only when it belongs to the recorded sequence. If the viewpoint changes, label that change explicitly rather than allowing it to enter through an inconsistent redraw.

Keep position separate from overlap. “Above the moon” describes placement in the view; it does not establish which object covers another. Where an edge interrupts another edge, record that interruption locally. Where no overlap is visible, leave the front-to-back relationship unspecified.

Give Each Sky Layer a Stable Visual Identity

Make a short inventory of the visible sky layers before assigning a disappearance order. Here, “layer” means a distinguishable part of the recorded sky. It need not correspond to a physical atmospheric layer or a separate sheet in a drawing application.

Identify each layer by something you can follow across successive states: its boundary, texture, color, transparency, or position relative to the eclipse and moon. Use neutral labels such as A and B alongside those descriptions. Keep the labels unchanged even when the appearance becomes faint.

For example, “A: a narrow textured band above the moon” would be an illustrative label, not an established feature of this scene. Add such a description only if the band is actually available to record. Do not fill the sky with extra bands merely to create a more elaborate sequence.

For each identified layer, note the following:

• Its visible extent and recognizable boundary.

• Whether it covers, reveals, or merely sits beside another visible feature.

• Whether underlying detail remains visible through it.

• Which identifying feature can still be followed as it changes.

Separate drawing layers can help preserve these distinctions. Krita’s official documentation describes layers as individually controllable parts of an image and explains that an upper paint layer can obscure all or part of one beneath it. That makes a layer stack useful for reconstructing overlap, provided its order follows the observed relationships. See Introduction to Layers and Masks (https://docs.krita.org/en/user_manual/layers_and_masks.html).

Keep the software arrangement subordinate to the record. Two visible sky regions may share one drawing layer; one complex sky region may require several. A file’s layer count should never become evidence for how many layers the scene contained.

Decide What “Disappears First” Means

Record two separate events: the first visible change and the first complete disappearance. They may belong to different layers. One layer might begin fading earlier but remain partly visible after another has vanished.

For this record, define complete disappearance as the first recorded state in which no recognizable part of that layer remains visible. This is a practical recording convention. It establishes a visible endpoint without claiming that the layer ceased to exist beyond the view.

Use precise verbs to describe the transition:

• “Fades” when the same region becomes progressively less visible.

• “Is covered” when another visible region advances across it.

• “Withdraws” when its boundary moves and its visible area contracts.

• “Leaves the view” when it passes beyond the picture boundary.

• “Is absent in the next recorded state” when the intervening change is unknown.

These descriptions answer different visual questions. If a moving boundary covers a layer, keep both the boundary’s movement and the covered region’s loss of visibility. If a layer becomes faint without a moving edge, do not add a sweeping transition for dramatic effect.

Also record what becomes visible in the vacated area. Is an already visible background exposed more fully? Does a neighboring region occupy the space? Is the resulting appearance unknown? A disappearance record is incomplete when it identifies what was lost but leaves an observable replacement undescribed.

Transparency masks offer a useful drawing analogy. Krita documents them as a way to hide selected parts of a layer without deleting the underlying image, including revealing material behind it. Use that distinction to keep “hidden from view” separate from “removed from the drawing.” See Transparency Masks (https://docs.krita.org/en/reference_manual/layers_and_masks/transparency_masks.html).

Build the Sequence Around Visible Changes

Start with the earliest available state, not an imagined fully intact sky. Label it “first recorded state.” Then add a new sketch whenever a meaningful visibility change occurs. Number the sketches in order without assigning elapsed seconds unless timing is actually available.

For each disappearance, aim to preserve the last state where the layer is recognizable and the first state where it is absent. Add an intermediate sketch only when an intermediate appearance is known. If the scene jumps directly between those states, retain the jump.

Use one short caption per transition. Identify the layer, the change, and what remains visible. “Layer A is no longer visible; layer B remains” is enough when those are the only established facts. Add a direction, texture change, or newly exposed region only when it can be supported by the record.

Continue through every available disappearance and any later reappearance. Do not stop after identifying the first layer if the rest of the sequence is known. End at the last available state; do not extend the scene into a cleared sky or a restored starting arrangement.

A digital timeline is optional. Krita’s timeline documentation organizes animated layers in rows and frame times in columns, and supports manually moving through frames to inspect changes. For this task, that structure can serve as a sequence viewer. Frame spacing chosen for convenient playback should be labeled as presentation timing when the scene’s duration is unknown. See Animation Timeline Docker (https://docs.krita.org/en/reference_manual/dockers/animation_timeline.html).

Use a Two-Pass Check to Resolve the Order

First, follow each layer individually from the opening state to the ending state. Note its earliest visible alteration and its first complete absence. Then compare those endpoints across layers. This separates a long fade from an earlier completed disappearance.

The following is an illustrative example only. It demonstrates the check without supplying missing facts about the eclipse scene:

1. State 1: layers A and B are both visible.

2. State 2: A becomes fainter; B appears unchanged.

3. State 3: A remains faintly visible; B is absent.

4. State 4: A is absent; B remains absent.

In that example, A changes first, while B disappears completely first. A caption saying only “A vanished first” would collapse two different observations into one inaccurate sequence.

For the second pass, compare neighboring sketches as whole images. Check whether the eclipse and giant moon retain their positions, sizes, and overlap relationships except where a change was recorded. Look especially at the moon’s upper edge and the space between the moon and eclipse: changes there can make a stable layer appear to shift.

Onion-skin comparison can help with this inspection. Krita describes onion skinning as displaying preceding and following frames over the current frame, usually with a tint. Use those overlays to compare boundaries, then turn them off to inspect the actual appearance of each state. The tinted overlays are comparison aids, not additional sky layers. See Onion Skin Docker (https://docs.krita.org/en/reference_manual/dockers/onion_skin.html).

Preserve an Incomplete Order Without Inventing the Missing Steps

Sometimes the available states establish only part of the order. If two layers are visible in one sketch and both absent in the next, their individual disappearance order is unresolved. Record “both absent by the next state; order unknown.” Do not split the transition into two invented events.

Likewise, if A is known to disappear before B but C cannot be placed, preserve that partial sequence. A useful record can say “A before B; C unresolved.” An honest gap is more informative than a polished sequence that adds unsupported changes.

Finish with a compact account naming the first complete disappearance, the later established order, and any unresolved interval. Keep the eclipse above the giant moon in the accompanying sketches, and preserve the final available state. The finished record should let a reader follow exactly what became invisible, when it became invisible relative to the other layers, and what remained in view.

Sources

• Introduction to Layers and Masks — Krita Manual (https://docs.krita.org/en/user_manual/layers_and_masks.html)

• Transparency Masks — Krita Manual (https://docs.krita.org/en/reference_manual/layers_and_masks/transparency_masks.html)

• Animation Timeline Docker — Krita Manual (https://docs.krita.org/en/reference_manual/dockers/animation_timeline.html)

• Onion Skin Docker — Krita Manual (https://docs.krita.org/en/reference_manual/dockers/onion_skin.html)