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NGC 7331, also known as Caldwell 30, is an unbarred spiral galaxy about 13.427 megaparsecs (43.79 million light-years) away in the constellation Pegasus. It was discovered by William Herschel on 6 September 1784.
The analysis highlights Supernovae, Galaxy Groups and Overview as prominent areas in the source structure around NGC 7331.
Source areas are shown by the number of related topics found in each part of the analysis. Use smaller areas too: they can reveal specialized angles and content gaps.
Smaller areas are not necessarily less important. They contain fewer connections in this analysis and can be useful for finding specialized angles or coverage gaps.
High-confidence facts extracted from structured source data. Use them as anchors for further research.
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The extracted context around NGC 7331 shows recurring relationship patterns in the source. For example, NGC 7331 → April, August, Four, Gates, GOTO, Howard, January, July, June, Kōichi Itagaki, Lick Observatory Supernova Search, LOSS, Milton Humason, NGC, Palomar Observatory, SN, Type Ib, Type II, Type II-L, Type IIn Another extracted example is NGC 7331 → Double, Erik Holmberg's, General Metagalactic Problems, Group, Holm, Inquiries, Multiple Galaxies Together, NGC, Study. Use these groups to spot repeated connection types before inspecting the individual relationships.
Use these terms to understand the vocabulary surrounding the topic, not as a checklist for keyword stuffing.
ngc 7331 galaxy spiral discovered type supernova also magnitude 13 supernovae pegasus sn observatory galaxies unbarred away appears structure milky
TTTA extracted 42 structured relationships around NGC 7331. Examples in this analysis include NGC 7331 → Apparent magnitude (V) → 10.4 and NGC 7331 → Apparent size (V) → 10.5′ × 3.7′. The table shows each extracted connection, where it came from and its confidence.
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| NGC 7331 | Apparent magnitude (V) | 10.4 | 1.00 | infobox |
| NGC 7331 | Apparent size (V) | 10.5′ × 3.7′ | 1.00 | infobox |
| NGC 7331 | Constellation | Pegasus | 1.00 | infobox |
| NGC 7331 | Declination | +34° 24′ 56.72″ | 1.00 | infobox |
| NGC 7331 | Distance | 43.79 ± 8.800 Mly (13.427 ± 2.698 Mpc) | 1.00 | infobox |
| NGC 7331 | Galactocentric velocity | 1,030±9 km/s | 1.00 | infobox |
| NGC 7331 | Heliocentric radial velocity | 816±1 km/s | 1.00 | infobox |
| NGC 7331 | Redshift | 0.002722±0.000003 | 1.00 | infobox |
| NGC 7331 | Right ascension | 22h 37m 04.0624s | 1.00 | infobox |
| NGC 7331 | Size | 146,250 ly (44.84 kpc) (diameter; 25.0 B-mag arcsec−2)[a] 112,920 ly × 55,316 ly (34.62 kpc × 16.96 kpc) (diameter; "total" magnitude)[a] | 1.00 | infobox |
| NGC 7331 | Type | SA(s)b; HII LINER | 1.00 | infobox |
| NGC 7331 | related to Galaxy Groups | NGC | 0.60 | section |
The concept neighborhoods around NGC 7331 bring nearby vocabulary together. In this analysis, examples include Galaxy, Spiral and Galaxies. Use the clusters to find adjacent concepts and terminology that may deserve separate research.
For NGC 7331, one of the stronger structural bridges in this analysis connects NGC 7331 with Supernovae. Bridges highlight paths between different parts of the map and can reveal research angles that are easy to miss in a flat list.
TTTA analyzes the structure around NGC 7331 to surface related topics, entities, relationships, concept neighborhoods and bridge connections. Use the map to explore areas such as Supernovae, Galaxy Groups & Overview, including less central topics that may reveal useful research gaps. Automatically extracted connections are research leads rather than rewritten encyclopedia content.
Source: Wikipedia — NGC 7331 · EN edition · Analysis: TopicsToTalkAbout