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HD 134606

star in the constellation Apus

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 13, 2026
Entity authorityQ22086879
Source-derived summary

HD 134606 is a yellow-hued star with a planetary system, positioned in the southern constellation of Apus. It is below the nominal limit for visibility with the naked eye, having an apparent visual magnitude of 6.86. Based upon an annual parallax shift of 37.3 mas, it is located 87.44 light-years away. The star appears to be moving further from the Earth with a heliocentric radial velocity of +1.9 km/s.

This is an evolving G-type subgiant star with a stellar classification of G6 IV and is not considered magnetically active, having a chromospheric activity index of −5.04. It has about the same mass as the Sun but is 25% more luminous. The photosphere is radiating energy at an effective temperature of 5,614 K. It has a higher than solar metallicity – a term astronomers use to describe the abundance of elements other than hydrogen and helium.

There is a companion star of spectral type M3V at a separation of ~1500 AU, designated L 72-1. Analysis of its light curve indicate it is itself a close binary.

Planetary system

The discovery of a planetary system orbiting HD 134606 was announced in 2011, following an eight-year survey carried out at the La Silla Observatory in Chile.

Editorial summary

“HD 134606” enters the record as star in the constellation Apus. Crown Archives preserves that source wording while asking what star, constellation and Apus can confirm, complicate or overturn.

Editorial reviewA concise reference frame for defining the subject, testing terminology and identifying the institution closest to the evidence. The current lead gives the account dated anchors—1500, 2011—that can be checked directly. The selected authority fields contribute no independent date. Its strongest next move is a source search built around star, constellation and Apus.
Editorial analysis

Why this record matters

“HD 134606” is worth following because a concise public description often conceals a longer documentary argument. Here, star, constellation and Apus provides the most credible route into that argument.

Evidence profile

Vocabulary and entity names are the principal evidence signals here, because they determine the precision of every later search. The source revision retrieved here is dated Sep 13, 2026. The linked authority identifier is Q22086879. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1500 and 2011.

Critical limits

Overview language is designed for orientation and should not be treated as a substitute for the evidence cited beneath it. The lead is largely declarative, so disagreement and counter-evidence require a deliberate search beyond the opening account. Authority statements aid reconciliation but still require their own references, qualifiers and ranks to be checked.

How to read it

Use the entry as an orientation point, then follow its citations and revision history. Names, dates and institutional relationships should be checked against the original record.

Best used for
  • Subject orientation
  • Search vocabulary
  • Locating named sources
Verify next

The closest primary source, responsible institution and strongest cited specialist reference.

Three-step research path

  1. Establish the record: confirm the title “HD 134606”, its source revision and the description used here.
  2. Expand the search: follow HD 134606 primary sources, HD 134606 archive and star research across catalogues and specialist indexes.
  3. Test the account: compare the strongest cited source with the responsible institution’s current record and note any disagreement.

Questions for further research

  1. Which source most directly establishes the central claim about “HD 134606”?
  2. Which cited source is closest to the event, object or claim?
  3. Which institution is responsible for the underlying evidence?
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Source & attribution

This entry incorporates text from HD 134606” on English Wikipedia. Contributors are listed in the page history. Text is available under the Creative Commons Attribution-ShareAlike 4.0 License. Selected authority identifiers and statements are retrieved from Wikidata under CC0; their references and qualifiers remain part of the verification path.