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NGC 262 je čočková galaxie a Seyfertova galaxie typu 2 nacházející se v souhvězdí Andromedy. Byla objevena 17. září 1885 Lewisem A. Swiftem. Tato galaxie má zdánlivou jasnost 13,1m a její úhlová velikost činí 1,1′ × 1,1′. Nachází se ve vzdálenosti přibližně 208 milionů světelných let.
The analysis highlights Charakteristiky, Význam pro výzkum and Overview as prominent areas in the source structure around NGC 262.
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 262 shows recurring relationship patterns in the source. For example, NGC 262 → Aktivita, NGC, Oblak, Obsahuje, Seyfertova, Seyfertovy, Slunce Another extracted example is NGC 262 → Aktivní, Markarjanova, NGC. 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 262 galaxie galaxií seyfertova typu přibližně vodíku sdss andromeda souhvězdí 17 září 1885 jasnost úhlová velikost 208 ultrafialovém spektra
TTTA extracted 28 structured relationships around NGC 262. Examples in this analysis include NGC 262 → Datum objevu → 17. září 1885 and NGC 262 → Deklinace → +31°57′25085″. The table shows each extracted connection, where it came from and its confidence.
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| NGC 262 | Datum objevu | 17. září 1885 | 1.00 | infobox |
| NGC 262 | Deklinace | +31°57′25085″ | 1.00 | infobox |
| NGC 262 | IRAS | IRAS 00461+3141 a IRAS F00460+3141 | 1.00 | infobox |
| NGC 262 | Jiná označení | NGC 262, PGC 2855, UGC 499, MCG +05-03-008, CGCG 501-20, 2MASX J00484711+3157249, IRAS 00461+3141, GALEXASC J004847.23+315726.3 | 1.00 | infobox |
| NGC 262 | Kupa galaxií | skupina NGC 266 skupina NGC 315 LGG 14 | 1.00 | infobox |
| NGC 262 | New General Catalogue | NGC 262 | 1.00 | infobox |
| NGC 262 | Objevitel | Lewis A. Swift | 1.00 | infobox |
| NGC 262 | Plošná jasnost | 13,2 | 1.00 | infobox |
| NGC 262 | Principal Galaxies Catalogue | PGC 2855 | 1.00 | infobox |
| NGC 262 | Rektascenze | 00h 48m 47,1414s | 1.00 | infobox |
| NGC 262 | Rudý posuv | 0,015034 ± 0,000013 | 1.00 | infobox |
| NGC 262 | Souhvězdí | Andromeda (lat. Andromeda) | 1.00 | infobox |
| NGC 262 | Typ | spirální galaxie, Seyfertova galaxie typu 2 a blazar | 1.00 | infobox |
| NGC 262 | Třída | SA(s)0/a: / Sy2 | 1.00 | infobox |
| NGC 262 | Uppsala General Catalogue | UGC 499 | 1.00 | infobox |
| NGC 262 | Vzdálenost | 208 M ly | 1.00 | infobox |
| NGC 262 | Zdánlivá magnituda (V) | 13,1 | 1.00 | infobox |
| NGC 262 | Úhlová velikost | 1,1′ × 1,1′ | 1.00 | infobox |
The concept neighborhoods around NGC 262 bring nearby vocabulary together. In this analysis, examples include Galaxií, Seyfertova and Typu. Use the clusters to find adjacent concepts and terminology that may deserve separate research.
For NGC 262, one of the stronger structural bridges in this analysis connects NGC 262 with Overview. 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 262 to surface related topics, entities, relationships, concept neighborhoods and bridge connections. Use the map to explore areas such as Charakteristiky, Význam pro výzkum & 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 262 · CS edition · Analysis: TopicsToTalkAbout
