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Lambda Andromedae

Lambda Andromedae 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 Lambda Andromedae rather than just read about it. In short: Lambda Andromedae, Latinized from λ Andromedae, also named Udkadua, is a binary star system in the northern constellation of Andromeda. At an estimated distance of approximately 84.6 light-years (25.9 parsecs) from Earth, it has an apparent visual magnitude of around +3.8.

Lambda Andromedae — main illustration
Lambda Andromedae — illustration

Key takeaways

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

Reference excerpt

Lambda Andromedae, Latinized from λ Andromedae, also named Udkadua, is a binary star system in the northern constellation of Andromeda. At an estimated distance of approximately 84.6 light-years (25.9 parsecs) from Earth, it has an apparent visual magnitude of around +3.8. This is bright enough to be seen with the naked eye. The system is drifting further away from the Sun with a radial velocity of +6.8 km/s.

Naming

This star represented the heel of the ancient Sumerian constellation Udkadua, "the storm demon with the gaping mouth". The IAU Working Group on Star Names approved the name Udkadua for the primary component of the system. Lambda Andromedae A on 8 May 2025 and it is now so entered in the IAU Catalog of Star Names. In traditional Arabic astronomy, the stars ι Andromedae, κ Andromedae, and λ Andromedae were known as Kaff al-Musalsala, the hand of the chained woman (i.e. Andromeda), and as Ra’s al-Nāqa, the head of the she-camel. In Chinese, 螣蛇 (Téng Shé), meaning Flying Serpent, refers to an asterism consisting of λ Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, κ Andromedae, ι Andromedae, and ψ Andromedae. Consequently, the Chinese name for λ Andromedae itself is 螣蛇十九 (Téng Shé shíjiǔ, English: the Nineteenth Star of Flying Serpent).

Properties

Lambda Andromedae is a single-lined spectroscopic binary with an orbital period of 20.52 days. The spectrum of the primary matches a stellar classification of G8 IV, meaning that it is an evolved star that is in the subgiant stage. The mass of this star is about 50% larger than that of the Sun, but it has expanded to around seven times the Sun's radius. It is radiating over 28 times the luminosity of the Sun from its outer envelope at an effective temperature of 4,800 K, giving it the characteristic yellow hue of a G-type star. This is an RS Canum Venaticorum variable and its brightness varies by 0.225 magnitudes, reaching a maximum of 3.70, with a period of 53.952 days. Such variability is theorized to occur because of tidal friction, which results in chromospheric activity. However, the orbit of this system is nearly circular, so the cause of this system's variability remains uncertain. The X-ray luminosity of this star, as measured by the ROSAT satellite, is 2.95×1030 erg/s. A magnetic field with an average strength of 21 G has been detected on this star, which is stronger than the field on the Sun. Starspots on the star's surface have been resolved with Doppler imaging. The secondary has a very low mass of about 0.1 M☉. It is most likely an L-type brown dwarf.

Evolution Many different spectral classes have been published for λ Andromedae, ranging from G6 to K1. Most sources give a luminosity class of III (giant) or IV (subgiant). Analysis of the physical properties of the star, including its temperature, luminosity, magnetic field, and stellar wind, show that it has recently experienced the first dredge-up and has begun to ascend the red giant branch although it still has a hot corona and is classified as a subgiant by some definitions.

References

External links http://www.alcyone-software.com/cgi-bin/search.pl?object=HR8961 Archived 2011-07-07 at the Wayback Machine Image Lambda Andromedae

Illustrations

Lambda Andromedae illustration
Lambda Andromedae: λ Andromedae in optical light
λ Andromedae in optical light
Lambda Andromedae: A light curve for Lambda Andromedae, plotted from Hipparcos data[16]
A light curve for Lambda Andromedae, plotted from Hipparcos data[16]

Worked examples

Example 1 — a first encounter with Lambda Andromedae

Start with the simplest possible case. Write down what Lambda Andromedae 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 Lambda Andromedae 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 Lambda Andromedae 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 Lambda Andromedae

In research
Lambda Andromedae 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 Lambda Andromedae 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
Lambda Andromedae is common in secondary-school and first-year university syllabi. It links to neighbouring topics Andromeda (constellation), Bayer objects, Bright Star Catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for Lambda Andromedae 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 Lambda Andromedae in 20 minutes

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

Frequently asked questions

What is Lambda Andromedae in simple terms?

Lambda Andromedae, Latinized from λ Andromedae, also named Udkadua, is a binary star system in the northern constellation of Andromeda. At an estimated distance of approximately 84.6 light-years (25.9 parsecs) from Earth, it has an apparent visual magnitude of around +3.8.

Why does Lambda Andromedae 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 Lambda Andromedae?

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 Lambda Andromedae.

Tags

  • Andromeda (constellation)
  • Bayer objects
  • Bright Star Catalogue objects
  • Durchmusterung objects
  • Flamsteed objects
  • G-type giants
  • G-type subgiants
  • Gliese and GJ objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • RS Canum Venaticorum variables
  • Spectroscopic binaries

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