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Psi Phoenicis

Psi Phoenicis 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 Psi Phoenicis rather than just read about it. In short: Psi Phoenicis (ψ Phoenicis) is a star in the constellation Phoenix. Its apparent magnitude varies from 4.3 to 4.5 with a period of about 30 days.

Psi Phoenicis — main illustration
Psi Phoenicis — illustration

Key takeaways

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

Reference excerpt

Psi Phoenicis (ψ Phoenicis) is a star in the constellation Phoenix. Its apparent magnitude varies from 4.3 to 4.5 with a period of about 30 days. It is visible to the naked eye. It is approximately 342 light years away based on parallax.

Psi Phoenicis is a red giant in the asymptotic branch with a spectral type of M4III, indicating it is an evolved star in the last evolutionary stage before becoming a white dwarf. In 1973 astronomer Olin J. Eggen discovered it is a variable star, varying in magnitude between 4.3 and 4.5 with an approximate period of 30 days. A more recent study identified two possible periods of 43.7 and 48.1 days, with amplitudes of 0.038 and 0.023 magnitudes. The star is classified as a semiregular variable, of no specific subtype. In 2001, Psi Phoenicis was observed by the VLT Interferometer with the test instrument VINCI. The observations, in combination with stellar atmospheric models, detected the limb darkening effect on the star's disk and found an angular diameter of 8.13±0.2 mas, corresponding to a stellar radius of 86±3 solar radii. From the radius and estimating an effective temperature of 3,550 K, a luminosity of 1,000 times the solar luminosity was calculated. A 2008 study reanalyzed the interferometric data with a new atmospheric model, finding an angular diameter of 10.15±0.15 mas and a radius of 85±1.6 R☉. By having directly measured distance, radius and luminosity, Psi Phoenicis was included in a list of 34 well characterized stars to be used as a reference. This program made the first measurement of the metallicity of Psi Phoenicis, showing it is a metal-poor star with only 5% the amount of iron of the Sun ([Fe/H] = −1.24±0.39). This value has a large uncertainty due to the difficulties in modeling the spectra of cool stars, which have strong molecular absorption. The evolutionary state and poorly constrained metallicity result in an uncertain mass of 1.0±0.4 M☉. Assuming a metallicity closer to solar, a mass of 1.3±0.2 M☉ is derived. Psi Phoenicis is considered a single star, and has no known companions. It has been considered a possible spectroscopic binary, including in the Hipparcos Catalogue, which stems from spectroscopic observations in 1919 which showed a possibly variable radial velocity. More recent data, however, showed the velocity to be constant.

References

Illustrations

Psi Phoenicis illustration
Psi Phoenicis: A light curve for Psi Phoenicis, plotted from Hipparcos data[11]
A light curve for Psi Phoenicis, plotted from Hipparcos data[11]

Worked examples

Example 1 — a first encounter with Psi Phoenicis

Start with the simplest possible case. Write down what Psi Phoenicis 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 Psi Phoenicis 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 Psi Phoenicis 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 Psi Phoenicis

In research
Psi Phoenicis 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 Psi Phoenicis 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
Psi Phoenicis is common in secondary-school and first-year university syllabi. It links to neighbouring topics Asymptotic-giant-branch stars, Bayer objects, Bright Star Catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for Psi Phoenicis 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 Psi Phoenicis in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Psi Phoenicis 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 Psi Phoenicis out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Psi Phoenicis in simple terms?

Psi Phoenicis (ψ Phoenicis) is a star in the constellation Phoenix. Its apparent magnitude varies from 4.3 to 4.5 with a period of about 30 days.

Why does Psi Phoenicis 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 Psi Phoenicis?

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 Psi Phoenicis.

Tags

  • Asymptotic-giant-branch stars
  • Bayer objects
  • Bright Star Catalogue objects
  • Durchmusterung objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • M-type giants
  • Phoenix (constellation)
  • Semiregular variable stars

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