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Zeta Pegasi

Zeta Pegasi is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Zeta Pegasi rather than just read about it. In short: Zeta Pegasi or ζ Pegasi, formally named Homam (), is a single star in the northern constellation of Pegasus. With an apparent visual magnitude of +3.4, this star is bright enough to be seen with the naked eye and is one of the brighter members of Pegasus.

Zeta Pegasi — main illustration
Zeta Pegasi — illustration

Key takeaways

  • Zeta Pegasi belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Zeta Pegasi to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Zeta Pegasi from memory before moving on to harder problems.

Reference excerpt

Zeta Pegasi or ζ Pegasi, formally named Homam (), is a single star in the northern constellation of Pegasus. With an apparent visual magnitude of +3.4, this star is bright enough to be seen with the naked eye and is one of the brighter members of Pegasus. Parallax measurements place it at a distance of around 204 light-years (62.7 parsecs) from the Sun.

Nomenclature ζ Pegasi (Latinised to Zeta Pegasi) is the star's Bayer designation. It bore the traditional name Homam, meaning "Man of High Spirit" or "Lucky Star of High Minded". In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN approved the name Homam for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names. In Chinese, 雷電 (Léi Diàn), meaning Thunder and Lightning, refers to an asterism consisting ζ Pegasi, ξ Pegasi, σ Pegasi, 55 Pegasi, 66 Pegasi and 70 Pegasi. Consequently, the Chinese name for ζ Pegasi itself is 雷電一 (Léi Diàn yī), "the First Star of Thunder and Lightning".

Properties

This star has a stellar classification of B8 V, which identifies it as a large B-type main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. The radius of this star is about four times that of the Sun. In 2007, John H. Goebel showed that Zeta Pegasi is a variable star, using data obtained from Gravity Probe B. It is a slowly pulsating B star that varies slightly in luminosity with a period of 22.952±0.804 hours, completing 1.04566 cycles per day. Zeta Pegasi is about 120 million years old and is rotating rapidly with a projected rotational velocity in the range of 140 to 210 km/s. The effective temperature of its outer envelope is around 12,300 K, giving it the characteristic blue-white glow of a B-type star. Zeta Pegasi has been examined for infrared excess that may indicate the presence of circumstellar matter, but none was found. This star does have two optical companions. The first is a magnitude 11.6 star at an angular separation of 68 arcseconds along a position angle of 139°, as of 1997. The second is an 11th magnitude star at a separation of 177 arcseconds with a position angle of 5°. Zeta Pegasi is not known to be a member of a stellar association.

References

Illustrations

Zeta Pegasi illustration
Zeta Pegasi: A light curve for Zeta Pegasi, adapted from Goebel (2007)[4]
A light curve for Zeta Pegasi, adapted from Goebel (2007)[4]

Worked examples

Example 1 — a first encounter with Zeta Pegasi

Start with the simplest possible case. Write down what Zeta Pegasi claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Zeta Pegasi before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Zeta Pegasi ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Zeta Pegasi

In research
Zeta Pegasi appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Zeta Pegasi in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Zeta Pegasi is common in secondary-school and first-year university syllabi. It links to neighbouring topics B-type main-sequence stars, Bayer objects, Bright Star Catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for Zeta Pegasi outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Zeta Pegasi in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Zeta Pegasi means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Zeta Pegasi out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Zeta Pegasi in simple terms?

Zeta Pegasi or ζ Pegasi, formally named Homam (), is a single star in the northern constellation of Pegasus. With an apparent visual magnitude of +3.4, this star is bright enough to be seen with the naked eye and is one of the brighter members of Pegasus.

Why does Zeta Pegasi matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Zeta Pegasi?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Zeta Pegasi.

Tags

  • B-type main-sequence stars
  • Bayer objects
  • Bright Star Catalogue objects
  • Durchmusterung objects
  • Flamsteed objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • Pegasus (constellation)
  • Slowly pulsating B-type stars
  • Stars with proper names

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