semiregular variable star
Let an agent describe semiregular variables by subclass, period, amplitude and observation, with sourced data.
Bundle → Layer → Finding → Questions Filled
4 bundles · 8 layers · 8 findings · 16 questions
Identity Which star.
Designation
Name.
Designation
Designation.
- What is the star variable designation? provenance
- Which subclass is it? definition
Type
Giant or supergiant.
Type
Star type.
- Is it a giant or supergiant, of which spectral type? definition
- How far away is it? measurement
Variability Light curve.
Period
Timescales.
Period
Period.
- What periods does it show? measurement
- Is there a long secondary period? provenance
Amplitude
Range.
Amplitude
Amplitude.
- What is the brightness range? measurement
- How irregular is it? definition
Physics Pulsation.
Mechanism
Pulsation modes.
Mechanism
Mechanism.
- What drives the pulsation, according to studies? provenance
- How certain is it? boundary
Evolution
Stage.
Evolution
Evolutionary stage.
- What evolutionary stage does it indicate? definition
- How does it relate to Miras? definition
Observing Contributing.
Visibility
Equipment.
Visibility
Visibility.
- Can it be observed with binoculars or small telescopes? boundary
- When is it best placed? measurement
Submit
Databases.
Submit
Submitting data.
- How can observations be submitted to variable star databases? action
- Which organisation runs them? provenance
Classifiers Filled
- Family
- Thing Registry
- Category
- Physical world and living systems
- Entry kind
- thing
- Plane
- PHY
- Domain
- PHY.SPC
- Other names and narrower kinds
- SRS semi-regular, Long Secondary Period variable, SRb semi-regular variable star, SRa semi-regular variable star, SRd semi-regular variable star, SRc semi-regular variable star
What it is Filled
A giant or supergiant pulsating variable star showing periodic brightness changes interrupted by irregularities, with periods from about 20 to over 2000 days; subclasses include SRa, SRb, SRc and SRd.
Why it exists Filled
Let an agent describe semiregular variables by subclass, period, amplitude and observation, with sourced data.
Distinguishing features Filled
- Semi-periodic pulsation
- Giants and supergiants
- Smaller amplitudes than Miras
- Common among red giants
What robots and AI may and may not do Filled
Must not
- Submit fabricated or unchecked observations to shared variable star databases.
- Misattribute observations to the wrong observer.
Only with a human decision
- Reclassifying a star in a catalogue that others rely on.
May
- Describe semiregular variables and their subclasses from variable star catalogues.
- Help observers log brightness estimates to the databases they contribute to.
Moral aspects Filled
- Amateur observers contribute much of the data and deserve credit.
- Shared databases depend on honest reporting.
Who is affected
- Observers
- Astronomers
Owners Filled
Steward
Nobody: held in common; variable star catalogues and observer databases record them.
Master systems
- General Catalogue of Variable Stars
- Variable star observer databases
Links to other meta-models Filled
parent
- Q1153690 - registry parent class
- Q353834 - registry parent class
related
- pulsating variable star - category
- Mira variable - long-period variables
- red giant - star type
- GCVS and VSX - catalogues
What else AI and robots need to interact with it Filled
Identity and identifiers required Filled
- Vercy registry: vr.tr.semiregular-variable-star
- Wikidata: Q1054411 (https://www.wikidata.org/wiki/Q1054411)
- GCVS designation: variable star names catalogue
Direct properties required Filled
- period: about 20-2000 days
- amplitude: up to about 2.5 magnitudes - visual
Recognition required Filled
- GCVS types SRa, SRb, SRc, SRd
- Irregular periodic light curves
- Long secondary periods in some
- Red giant or supergiant stars varying in brightness over weeks to years.
Capabilities and actions required Filled
- classify by subclass
- record light curves
- submit observations to databases
- compare with Mira variables
Hazards and failure modes required Filled
- Misclassifying subtype
- Overinterpreting sparse data
Standards and interfaces required Filled
- IAU variable star nomenclature
Context of use required Filled
- Studying late stellar evolution and pulsation.
- SRa
- SRb
- SRc (supergiants)
- SRd (yellow giants)
- stars with long secondary periods
Sources Filled
- Wikidata item Q1054411: semiregular variable star - identity and sense of the item
- Wikipedia: Semiregular variable star - general description of the item
Open questions
- Should subclasses be separate entries?
- How should VSX data be linked?
- How should long secondary periods be explained?
Machine files
Provenance
thing registry research (pass 2) · unreviewed
Built from: models/things/publications/thing-q1054411/spec.json