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Open cluster family

Open cluster family 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 Open cluster family rather than just read about it. In short: In astronomy, an open cluster family is a group of approximately coeval (age range ∼ {\displaystyle \sim } 30 Myr) young open star clusters located in a relatively small region of the Galactic disk (radius ∼ {\displaystyle \sim } 250 pc). Introduction Open clusters do not form in isolation but in complexes (Efremov 1978), within star forming regions.

Key takeaways

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

Reference excerpt

In astronomy, an open cluster family is a group of approximately coeval (age range ∼ {\displaystyle \sim } 30 Myr) young open star clusters located in a relatively small region of the Galactic disk (radius ∼ {\displaystyle \sim } 250 pc).

Introduction Open clusters do not form in isolation but in complexes (Efremov 1978), within star forming regions. When age, spatial distribution, and kinematics are taken into account simultaneously, a significant number of known young open clusters are found in groups. Piskunov et al. (2006) found evidence for four open cluster complexes (OCCs) of different ages containing up to a few tens of clusters. The existence of at least five dynamical families of young open clusters in the Milky Way disk has been confirmed using statistical analysis by de la Fuente Marcos and de la Fuente Marcos (2008). They are, in order of increasing distance: Orion, Scutum-Sagittarius, Cygnus, Scorpius, and Cassiopeia-Perseus. These families are associated to the Galactic spiral structure, they are short-lived as they disperse in a relatively short timescale and they are progenitors of classical superclusters, moving groups, and stellar streams (de la Fuente Marcos & de la Fuente Marcos 2008). The Cassiopeia-Perseus open cluster family is located 2 kpc from the Sun between the constellations of Cassiopeia and Perseus, embedded in the Perseus spiral arm (de la Fuente Marcos & de la Fuente Marcos 2009). The structure roughly defines a plane that is inclined almost 30° with respect to the plane of the Milky Way. It has a diameter of about 600 pc and includes 10 to 20 members. Most candidate members are located below the galactic disk and moving away from it. It started to form about 20 to 40 Myr (1 Myr = 106 yr) ago.

See also Stellar association Moving groups Open cluster Open cluster remnant Star cluster

References Efremov, Y. N. 1978, Soviet Astronomy Letters, 4, 66-69 (ADS entry) de la Fuente Marcos, Raúl; & de la Fuente Marcos, Carlos (2008), Astrophysical Journal, 672, 342-351 (ADS entry) de la Fuente Marcos, Raúl; & de la Fuente Marcos, Carlos (2009), New Astronomy, 14, 180-195 (ADS entry) Piskunov, A. E., Kharchenko, N. V., Röser, S., Schilbach, E., & Scholz, R.-D. 2006, Astronomy and Astrophysics, 445, 545-565 (ADS entry)

Worked examples

Example 1 — a first encounter with Open cluster family

Start with the simplest possible case. Write down what Open cluster family 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 Open cluster family 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 Open cluster family 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 Open cluster family

In research
Open cluster family 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 Open cluster family 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
Open cluster family is common in secondary-school and first-year university syllabi. It links to neighbouring topics Open clusters, Star clusters, so understanding it makes those chapters shorter.
In everyday life
Look for Open cluster family 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 Open cluster family in 20 minutes

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

Frequently asked questions

What is Open cluster family in simple terms?

In astronomy, an open cluster family is a group of approximately coeval (age range ∼ {\displaystyle \sim } 30 Myr) young open star clusters located in a relatively small region of the Galactic disk (radius ∼ {\displaystyle \sim } 250 pc). Introduction Open clusters do not form in isolation but in c…

Why does Open cluster family 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 Open cluster family?

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 Open cluster family.

Tags

  • Open clusters
  • Star clusters

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