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HD 98649

star in the constellation Crater

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionOct 15, 2025
Entity authorityQ5629385
Source-derived summary

HD 98649 is a star with an orbiting exoplanet in the southern Crater constellation. Based on parallax measurements, it is situated at a distance of 137.5 light years from the Sun. The system is drifting further away with a heliocentric radial velocity of 4.3 km/s. With an apparent visual magnitude of +8.00, it is too faint to be viewed with the naked eye. The system has a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.24″·yr−1.

The spectrum of HD 98649 presents as an ordinary G-type main-sequence star with a stellar classification of G3/5V. It is around 4.4 billion years old and is spinning slowly with a rotation period of roughly 27 days. The star is similar to the Sun, having nearly the same size, mass, and luminosity. It is considered a solar analog. The level of magnetic activity in the chromosphere is minimal.

Planetary system

From 1998 to 2012, the star was under observance from the CORALIE echelle spectrograph at La Silla Observatory.

Editorial summary

The public source identifies “HD 98649” as star in the constellation Crater. This brief keeps that definition visible, then builds a research path around star, constellation and Crater.

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—1998, 2012—that can be checked directly. The selected authority fields contribute no independent date. Its value is orientation rather than verdict, with star, constellation and Crater providing the first useful test.
Editorial analysis

Why this record matters

A short description can identify a subject without explaining its stakes. For “HD 98649”, the useful work is to connect “star in the constellation Crater” to the records capable of establishing context and consequence.

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 Oct 15, 2025. The linked authority identifier is Q5629385. None of the 0 selected statements returned an explicit reference. The first chronological checks are 1998 and 2012.

Critical limits

A concise general-reference account can conceal disagreements about scope, terminology or the weight assigned to individual sources. 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 98649”, its source revision and the description used here.
  2. Expand the search: follow HD 98649 primary sources, HD 98649 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 98649”?
  2. What terminology or title could unlock a more precise catalogue search?
  3. Which institution is responsible for the underlying evidence?
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Source & attribution

This entry incorporates text from HD 98649” 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.