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1156 Kira

asteroid

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 5, 2026
Entity authorityQ136581
Source-derived summary

1156 Kira, provisional designation 1928 DA, is a stony background asteroid from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 22 February 1928, by German astronomer Karl Reinmuth at Heidelberg Observatory in southwest Germany. Any reference of its name to a person or occurrence is unknown.

Orbit and classification

Kira is not a member of any known asteroid family and belongs to the main belt's background population. At the present epoch, however, it orbits within the region of the Flora family.

This asteroid orbits the Sun in the inner main-belt at a distance of 2.1–2.3 AU once every 3 years and 4 months (1,222 days). Its orbit has an eccentricity of 0.05 and an inclination of 1° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Heidelberg.

Physical characteristics

Kira is an assumed stony S-type asteroid.

Rotation period

Several rotational lightcurves of Kira have been obtained from photometric observations since 2007.

Editorial summary

Begin with the source’s own compact description: “1156 Kira” is asteroid. The dossier treats that line as a proposition to test through Kira and asteroid, not as a finished interpretation.

Editorial reviewA practical starting point whose main value is the path it opens into stronger specialist and primary sources. The current lead gives the account dated anchors—1156, 1928, 2007—that can be checked directly. The selected authority fields contribute no independent date. For this dossier, Kira and asteroid is the immediate research focus.
Editorial analysis

Why this record matters

The phrase “asteroid” supplies a clear boundary for inquiry. It also exposes the unanswered questions: who defined that boundary, when it became stable and which sources sit outside it.

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 5, 2026. The linked authority identifier is Q136581. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1156, 1928 and 2007.

Critical limits

The absence of detail may reflect summary conventions rather than a lack of surviving documentation. The source lead contains qualifying language; that uncertainty should survive quotation, summary and reuse. 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 “1156 Kira”, its source revision and the description used here.
  2. Expand the search: follow 1156 Kira primary sources, 1156 Kira archive and Kira 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 “1156 Kira”?
  2. Which cited source is closest to the event, object or claim?
  3. What terminology or title could unlock a more precise catalogue search?
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Source & attribution

This entry incorporates text from 1156 Kira” 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.