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(415029) 2011 UL21

an Apollo class asteroid

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 6, 2026
Entity authorityQ4622750
Source-derived summary

(415029) 2011 UL21 is an Apollo-class potentially hazardous asteroid discovered on 17 October 2011, by the Catalina Sky Survey project. The asteroid is estimated to have a diameter of 2.5 kilometres (1.6 mi). It was rated at Torino scale 1 on 27 October 2011, with an observation arc of 9.6 days. 2011 UL21 is the largest asteroid ever to be rated above a 0 on the Torino scale.

Description

2011 UL21 briefly had about a 1 in a million chance of impacting in 2029. Its cumulative impact probability dropped to 1 in 71 million by 2 November 2011 when the observation arc reached 15 days. It was removed from the Sentry risk table on 4 November 2011 when all impact scenarios for the next 100 years or more were ruled out. During 2029, the closest approach to Earth is 1.6 AU. Palomar Observatory precovery images from 1989 and 1990 have extended the observation arc to 22 years.

With an absolute magnitude of 15.8, it is one of the brightest and therefore largest potentially hazardous asteroids (PHA) detected since (242450) 2004 QY2. The next largest PHA (based on absolute magnitude) discovered in 2011 is 2011 WO41 with an absolute magnitude of 16.8.

Editorial summary

Begin with the source’s own compact description: “(415029) 2011 UL21” is an Apollo class asteroid. The dossier treats that line as a proposition to test through UL21, Apollo and class, not as a finished interpretation.

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—2011, 2029, 1989, 1990—that can be checked directly. The selected authority fields contribute no independent date. For this dossier, UL21, Apollo and class is the immediate research focus.
Editorial analysis

Why this record matters

The phrase “an Apollo class 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

Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Sep 6, 2026. The linked authority identifier is Q4622750. None of the 0 selected statements returned an explicit reference. The first chronological checks are 2011, 2029, 1989 and 1990.

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.

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

Three-step research path

  1. Establish the record: confirm the title “(415029) 2011 UL21”, its source revision and the description used here.
  2. Expand the search: follow (415029) 2011 UL21 primary sources, (415029) 2011 UL21 archive and UL21 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

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Source & attribution

This entry incorporates text from (415029) 2011 UL21” 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.