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Research draft

planetary system

vr.tr.planetary-system · PHY.SPC

Let an agent handle planetary systems by host star, members, architecture, discovery method and habitability, with sourced catalogue data.

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 handle planetary systems by host star, members, architecture, discovery method and habitability, with sourced catalogue data.

A set of gravitationally bound non-stellar objects, such as planets, dwarf planets, moons, asteroids and comets, orbiting a star or star system; the Solar System is one example, and thousands of exoplanet systems are known.

What it is for: Understanding planets and their origins.

It can be list known planets of a system; compare system architectures; explain detection methods; discuss habitable zones with sources.

Distinguishing features

Bound to a star

Diverse architectures

Mostly detected indirectly

Formed from protoplanetary disks

What it looks like

A star with orbiting planets; mostly known from indirect measurements.

How it is recognised

Host star and planet designations such as b, c, d

Detection by transit, radial velocity or imaging

Star clusters are not planetary systems

Related models

is a kind of - category

gravitationally bound system

orbits - host

star

contains - member

planet

forms from - origin

protoplanetary disk

In practice

Families and kinds

the Solar System

multi-planet exoplanet systems

circumbinary systems

pulsar planet systems

systems with debris disks

Identifiers

exoplanet catalogue host name plus letter designations

Standards and regulation

IAU naming conventions for exoplanets

Failure modes and hazards

Presenting candidates as confirmed planets

Overstating habitability

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.

System Which system.

Hosts identify systems.

Host

Star.

Host

Host star.

  1. Which star hosts the system, and how far is it? provenance
  2. What type of star is it? definition

Members

Planets.

Members

Members.

  1. Which planets are confirmed, according to which archive? provenance
  2. Which are candidates? boundary
Architecture Layout.

Architectures vary.

Orbits

Periods and distances.

Orbits

Orbits.

  1. What are the orbital periods and distances? measurement
  2. Are there resonances? definition

Comparison

Solar System.

Comparison

Comparison.

  1. How does it compare with the Solar System? definition
  2. What is unusual about it? provenance
Detection Methods.

Methods shape knowledge.

Method

Transit, RV.

Method

Detection method.

  1. Which method detected the planets? provenance
  2. What biases does the method have? boundary

Confirmation

Status.

Confirmation

Confirmation.

  1. Has the detection been confirmed independently? provenance
  2. Which paper reported it? provenance
Habitability Life potential.

Claims need care.

Zone

Habitable zone.

Zone

Habitable zone.

  1. Does any planet orbit in the habitable zone? boundary
  2. Which definition of the zone is used? definition

Claims

Biosignatures.

Claims

Life claims.

  1. Are there any claimed biosignatures, and are they confirmed? boundary
  2. Which sources discuss them? provenance

What the second pass must settle

  • Should each system be a separate entry?
  • How should exoplanet archives be linked?
  • How should candidate status be shown?