Q85580481

Thing t_tauri_type_star Q85580481

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Q85580481

Summary

Q85580481 is a T Tauri-type star^[1].

Key Facts

Q85580481's instance of is recorded as T Tauri-type star^[2].
Q85580481's constellation is recorded as Perseus^[3].
Q85580481's spectral class is recorded as M4^[4].
Q85580481's part of is recorded as IC 348^[5].
Q85580481's catalog code is recorded as Cl* IC 348 LRL 138^[6].
Q85580481's catalog code is recorded as 2MASS J03444508+3214130^[7].
Q85580481's catalog code is recorded as CXOPZ 179^[8].
Q85580481's catalog code is recorded as Cl* IC 348 CPS 101^[9].
Q85580481's catalog code is recorded as CXOPZ J034445.1+321414^[10].
Q85580481's catalog code is recorded as SSTc2d J034445.1+321413^[11].
Q85580481's catalog code is recorded as [PSZ2003] J034445.1+321413^[12].
Q85580481's catalog code is recorded as CXOU J034445.1+321414^[13].
Q85580481's catalog code is recorded as [BNM2013] 32.03 395^[14].
Q85580481's catalog code is recorded as Gaia DR2 216705186260474112^[15].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.64'}^[16].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.36'}^[17].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+23.018'}^[18].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.661'}^[19].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.954'}^[20].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.564'}^[21].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.147'}^[22].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.560'}^[23].
Q85580481's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.7695'}^[24].
Q85580481's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.6735'}^[25].
Q85580481's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+13.093452000'}^[26].

⭐ Popularity Graph

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Quick Facts

Instance of T Tauri-type star

Part of IC 348

Properties

Apparent magnitude unit: 1, amount: +19.64, unit: 1, amount: +17.36, unit: 1, amount: +23.018, unit: 1, amount: +20.661, unit: 1, amount: +17.954, unit: 1, amount: +13.564, unit: 1, amount: +12.147, unit: 1, amount: +11.560, unit: 1, amount: +18.7695

Catalog code Cl* IC 348 LRL 138, 2MASS J03444508+3214130, CXOPZ 179, Cl* IC 348 CPS 101, CXOPZ J034445.1+321414, SSTc2d J034445.1+321413, [PSZ2003] J034445.1+321413, CXOU J034445.1+321414, [BNM2013] 32.03 395, Gaia DR2 216705186260474112

Constellation Perseus

Declination unit: www.wikidata.org, amount: +32.23699242183260

Declination component of proper motion unit: www.wikidata.org, amount: -6.942

Effective temperature unit: www.wikidata.org, amount: +3319

Epoch J2000.0

Imported from wholeness_audit_2026-05-02_v2

Parallax unit: www.wikidata.org, amount: +2.6735

Radial velocity unit: www.wikidata.org, amount: +13.093452000, unit: www.wikidata.org, amount: +15.549070, unit: www.wikidata.org, amount: +15.824127, unit: www.wikidata.org, amount: +15.688164, unit: www.wikidata.org, amount: +15.963221, unit: www.wikidata.org, amount: +15.438743, unit: www.wikidata.org, amount: +15.713799, unit: www.wikidata.org, amount: +13.093452, unit: www.wikidata.org, amount: +13.368510

Right ascension unit: www.wikidata.org, amount: +56.18789291838500

Right ascension component of proper motion unit: www.wikidata.org, amount: +3.416

Spectral class M4

Stellar rotational velocity unit: www.wikidata.org, amount: +31.48

Surface gravity unit: www.wikidata.org, amount: +7000

External References (2)

Gaia id 216705186260474112

Simbad id Cl* IC 348 LRL 138

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

[2] ↑ Q85580481 — instance of (P31): T Tauri-type star. SIMBAD. wikidata.org.
[3] ↑ Q85580481 — constellation (P59): Perseus. wikidata.org.
[4] ↑ Q85580481 — spectral class (P215): M4. Deep MIPS observations of the IC 348 nebula: constraints on the evolutionary state of anemic circumstellar disks and the primordial-to-debris disk transition. wikidata.org.
[5] ↑ Q85580481 — part of (P361): IC 348. SIMBAD. wikidata.org.
[6] ↑ Q85580481 — catalog code (P528): Cl* IC 348 LRL 138. SIMBAD. wikidata.org.
[7] ↑ Q85580481 — catalog code (P528): 2MASS J03444508+3214130. SIMBAD. wikidata.org.
[8] ↑ Q85580481 — catalog code (P528): CXOPZ 179. SIMBAD. wikidata.org.
[9] ↑ Q85580481 — catalog code (P528): Cl* IC 348 CPS 101. SIMBAD. wikidata.org.
[10] ↑ Q85580481 — catalog code (P528): CXOPZ J034445.1+321414. SIMBAD. wikidata.org.
[11] ↑ Q85580481 — catalog code (P528): SSTc2d J034445.1+321413. SIMBAD. wikidata.org.
[12] ↑ Q85580481 — catalog code (P528): [PSZ2003] J034445.1+321413. SIMBAD. wikidata.org.
[13] ↑ Q85580481 — catalog code (P528): CXOU J034445.1+321414. SIMBAD. wikidata.org.
[14] ↑ Q85580481 — catalog code (P528): [BNM2013] 32.03 395. SIMBAD. wikidata.org.
[15] ↑ Q85580481 — catalog code (P528): Gaia DR2 216705186260474112. SIMBAD. wikidata.org.
[16] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+19.64'}. TheSpitzerc2d Survey of Weak‐Line T Tauri Stars. II. New Constraints on the Timescale for Planet Building. wikidata.org.
[17] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+17.36'}. TheSpitzerc2d Survey of Weak‐Line T Tauri Stars. II. New Constraints on the Timescale for Planet Building. wikidata.org.
[18] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+23.018'}. Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
[19] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+20.661'}. Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
[20] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+17.954'}. Pre-main-sequence isochrones – II. Revising star and planet formation time-scales. wikidata.org.
[21] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+13.564'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
[22] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+12.147'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
[23] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+11.560'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
[24] ↑ Q85580481 — apparent magnitude (P1215): {'unit': '1', 'amount': '+18.7695'}. Gaia Data Release 2. wikidata.org.
[25] ↑ Q85580481 — parallax (P2214): {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.6735'}. Gaia Data Release 2. wikidata.org.
[26] ↑ Q85580481 — radial velocity (P2216): {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+13.093452000'}. IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.

Class ancestry

[1] ↑ Q85580481 is an instance of T Tauri-type star (Q6232) [P31, primary]. Wikidata. wikidata.org.

📑 Cite this page

Use these citations when quoting this entity in research, articles, AI prompts, or wherever provenance matters. We aggregate Wikidata + Wikipedia + authoritative open-data sources; the stitched, scored, cross-referenced view is what 4ort.xyz contributes.

APA 4ort.xyz Knowledge Graph. (2026). Q85580481. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85580481

MLA “Q85580481.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85580481.

BibTeX

@misc{4ortxyz_q85580481_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85580481}}, year = {2026}, url = {https://4ort.xyz/entity/q85580481}, note = {Accessed: 2026-05-07}}

LLM prompt

According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85580481 — https://4ort.xyz/entity/q85580481 (retrieved 2026-05-07)

Canonical URL: https://4ort.xyz/entity/q85580481 · Last refreshed: May 7, 2026