Q84210445

Thing orion_variable Q84210445

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Q84210445

Summary

Q84210445 is an Orion variable^[1].

Key Facts

Q84210445's instance of is recorded as Orion variable^[2].
Q84210445's instance of is recorded as eruptive variable star^[3].
Q84210445's instance of is recorded as near-infrared source^[4].
Q84210445's instance of is recorded as astrophysical X-ray source^[5].
Q84210445's instance of is recorded as young stellar object^[6].
Q84210445's constellation is recorded as Orion^[7].
Q84210445's spectral class is recorded as M0.9^[8].
Q84210445 is part of Q84210325^[9].
Q84210445's catalog code is recorded as 2MASS J05360110-0615314^[10].
Q84210445's catalog code is recorded as [MGM2012] 991^[11].
Q84210445's catalog code is recorded as SDSS J053601.10-061531.5^[12].
Q84210445's catalog code is recorded as SOXS 386^[13].
Q84210445's catalog code is recorded as Gaia DR2 3017165532751368960^[14].
Q84210445's catalog code is recorded as V393 Ori^[15].
Q84210445's catalog code is recorded as TIC 388935437^[16].
Q84210445's catalog code is recorded as Gaia DR3 3017165532751368960^[17].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.604'}^[18].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.498'}^[19].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.613'}^[20].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.849'}^[21].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.793'}^[22].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.027'}^[23].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.535'}^[24].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.177'}^[25].
Q84210445's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.44'}^[26].

Body

Definition and Type

Recorded instance of include Orion variable^[2], eruptive variable star^[3], near-infrared source^[4], astrophysical X-ray source^[5], and young stellar object^[6].

Use and Application

Q84210445 is part of Q84210325^[9].

⭐ Popularity Graph

0/100 long tail

Quick Facts

Instance of Orion variable, eruptive variable star, near-infrared source, astrophysical X-ray source, young stellar object

Part of LDN 1641

Properties

Apparent magnitude unit: 1, amount: +15.604, unit: 1, amount: +13.498, unit: 1, amount: +16.613, unit: 1, amount: +15.849, unit: 1, amount: +14.793, unit: 1, amount: +18.027, unit: 1, amount: +13.535, unit: 1, amount: +12.177, unit: 1, amount: +11.44, unit: 1, amount: +11.050, unit: 1, amount: +14.830334

Catalog code 2MASS J05360110-0615314, [MGM2012] 991, SDSS J053601.10-061531.5, SOXS 386, Gaia DR2 3017165532751368960, V393 Ori, TIC 388935437, Gaia DR3 3017165532751368960

Constellation Orion

Declination unit: www.wikidata.org, amount: -6.25873655205

Declination component of proper motion unit: www.wikidata.org, amount: +0.436

Distance from earth unit: www.wikidata.org, amount: +395.304

Effective temperature unit: www.wikidata.org, amount: +3989

Epoch J2000.0

Imported from wholeness_audit_2026-05-02_v2

Parallax unit: www.wikidata.org, amount: +2.5297

Radial velocity unit: www.wikidata.org, amount: +23.862301

Right ascension unit: www.wikidata.org, amount: +84.0046003

Right ascension component of proper motion unit: www.wikidata.org, amount: +0.217

Spectral class M0.9

Stellar rotational velocity unit: www.wikidata.org, amount: +11.539

Surface gravity unit: www.wikidata.org, amount: +34435

External References (2)

Gaia id 3017165532751368960

Simbad id V* V393 Ori

🏷️ Also known as

ru V393 Ориона

References

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

Direct Wikidata claims

[2] ↑ Q84210445 — instance of (P31): Orion variable. SIMBAD. wikidata.org.
[3] ↑ Q84210445 — instance of (P31): eruptive variable star. SIMBAD. wikidata.org.
[4] ↑ Q84210445 — instance of (P31): near-infrared source. SIMBAD. wikidata.org.
[5] ↑ Q84210445 — instance of (P31): astrophysical X-ray source. SIMBAD. wikidata.org.
[6] ↑ Q84210445 — instance of (P31): young stellar object. SIMBAD. wikidata.org.
[7] ↑ Q84210445 — constellation (P59): Orion. wikidata.org.
[8] ↑ Q84210445 — spectral class (P215): M0.9. The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. wikidata.org.
[9] ↑ Q84210445 — part of (P361): Q84210325. SIMBAD. wikidata.org.
[10] ↑ Q84210445 — catalog code (P528): 2MASS J05360110-0615314. SIMBAD. wikidata.org.
[11] ↑ Q84210445 — catalog code (P528): [MGM2012] 991. SIMBAD. wikidata.org.
[12] ↑ Q84210445 — catalog code (P528): SDSS J053601.10-061531.5. SIMBAD. wikidata.org.
[13] ↑ Q84210445 — catalog code (P528): SOXS 386. SIMBAD. wikidata.org.
[14] ↑ Q84210445 — catalog code (P528): Gaia DR2 3017165532751368960. SIMBAD. wikidata.org.
[15] ↑ Q84210445 — catalog code (P528): V393 Ori. SIMBAD. wikidata.org.
[16] ↑ Q84210445 — catalog code (P528): TIC 388935437. SIMBAD. wikidata.org.
[17] ↑ Q84210445 — catalog code (P528): Gaia DR3 3017165532751368960. SIMBAD. wikidata.org.
[18] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+15.604'}. The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. wikidata.org.
[19] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+13.498'}. The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function. wikidata.org.
[20] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+16.613'}. The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
[21] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+15.849'}. The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
[22] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+14.793'}. The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
[23] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+18.027'}. The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
[24] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+13.535'}. The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III baryon oscillation spectroscopic survey. wikidata.org.
[25] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+12.177'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
[26] ↑ Q84210445 — apparent magnitude (P1215): {'unit': '1', 'amount': '+11.44'}. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.

Class ancestry

[1] ↑ Q84210445 is an instance of Orion variable (Q1352333) [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). Q84210445. Retrieved May 7, 2026, from https://4ort.xyz/entity/q84210445

MLA “Q84210445.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q84210445.

BibTeX

@misc{4ortxyz_q84210445_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q84210445}}, year = {2026}, url = {https://4ort.xyz/entity/q84210445}, note = {Accessed: 2026-05-07}}

LLM prompt

According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q84210445 — https://4ort.xyz/entity/q84210445 (retrieved 2026-05-07)

Canonical URL: https://4ort.xyz/entity/q84210445 · Last refreshed: May 7, 2026