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Research draft

nova

vr.tr.nova · PHY.SPC

Let an agent describe novae by designation, type, light curve and visibility, and separate them from supernovae.

Thing Registry Physical world and living systems

Research draft, second pass

A second pass drafted this model: the structure a model of this thing needs, and what is known about it in the world. The line under this one says how the second half was obtained - researched against sources, or recalled without web access, in which case nothing here was read anywhere and every claim is a lead to verify. Unreviewed either way.

written by Claude from model knowledge without web access - no source was read, every claim is a lead to verify

Researched by: Claude

Purpose and description

Let an agent describe novae by designation, type, light curve and visibility, and separate them from supernovae.

A sudden brightening of a star caused by a thermonuclear explosion on the surface of a white dwarf accreting matter from a companion, after which it fades; recurrent novae repeat.

What it is for: Novae reveal binary evolution and produce some elements.

It can be discover and observe it; record light curves; study the binary system; alert observers.

Distinguishing features

Surface explosion on a white dwarf

Star survives

Recurrent in some systems

Different from supernova

What it looks like

A new star appearing for days to months, then fading.

Physical character

brightening: 8-15 magnitudes

decline time: days to months time

How it is recognised

Sudden brightening in a previously faint star

Designations such as Nova Cygni with year

Supernovae are far more energetic

Related models

occurs on - host

white dwarf

is part of - system

binary star

is confused with - much larger

supernova

is a kind of - category

variable star

In practice

Families and kinds

classical novae

recurrent novae

symbiotic novae

fast and slow novae

micronovae

Identifiers

nova designation Nova plus constellation plus year or variable star name names

Standards and regulation

IAU nomenclature

Failure modes and hazards

Confusing with supernovae

Overhyping predicted novae

Also called

recurrent novamicronovasupernova impostorsymbiotic novafast novaeslow novaefailed supernova

Where this came from

wikidata · CC0 1.0

Drafted structure

Bundle to layer to finding to question, as the second pass will find it: 4 bundles · 8 layers · 8 findings · 16 questions.

Identity Which nova.

Names and systems.

Designation

Name.

Designation

Designation.

  1. What is its designation? provenance
  2. When was it discovered? provenance

Type

Classical or recurrent.

Type

Nova type.

  1. Is it classical or recurrent? definition
  2. What kind of binary hosts it? definition
Light curve Brightness over time.

Light curves characterise novae.

Peak

Maximum brightness.

Peak

Peak brightness.

  1. How bright did it get, and when? measurement
  2. How fast did it fade? measurement

Data

Observations.

Data

Data sources.

  1. Which observers recorded it? provenance
  2. Where are data archived? provenance
Physics Why it happens.

Mechanism explains recurrence.

Mechanism

Accretion and ignition.

Mechanism

Mechanism.

  1. How does the explosion occur? definition
  2. How often might it recur? measurement

Products

Ejecta.

Products

Ejecta.

  1. What material does it eject? measurement
  2. What does it contribute chemically? definition
Observing Seeing it.

Observers want to see novae.

Visibility

Naked eye?

Visibility

Visibility.

  1. Is it visible to the naked eye, and where? action
  2. For how long? measurement

Predictions

Expected novae.

Predictions

Predictions.

  1. Is an eruption predicted, and how reliably? boundary
  2. Which source? provenance

What the second pass must settle

  • Should novae be instances?
  • How should light curves be linked?
  • How should predictions be communicated?