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NEODyS

NEODyS 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 NEODyS rather than just read about it. In short: NEODyS (Near Earth Objects Dynamic Site) is an Italian service that provides information on near-Earth objects with a Web-based interface. It is based on a continually and (almost) automatically maintained database of near earth asteroid orbits.

Key takeaways

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

Reference excerpt

NEODyS (Near Earth Objects Dynamic Site) is an Italian service that provides information on near-Earth objects with a Web-based interface. It is based on a continually and (almost) automatically maintained database of near earth asteroid orbits. This site provides a number of services to the NEO community. The main service is an impact monitoring system (CLOMON2) of all near-Earth asteroids covering a period until the year 2100.

Services Risk Page: One of the most important services is the production of a Risk Page where 1128 NEOs with probabilities of hitting the Earth greater of 10−11 from now until 2100 are shown in a Risk list. In the table of the Risk list the NEOs are divided into "Special", as it is the case of 101955 Bennu; "Observable", objects which are presently observable and which critically need a follow-up in order to improve their orbit; "Possible recovery", objects which are not visible at present, but which are possible to recover in the near future; "Lost", objects which have an absolute magnitude (H) brighter than 25 but which are virtually lost, being their orbit too uncertain; and "Small", objects with an absolute magnitude fainter than 25 and, even if they are "lost", they are considered too small to result in heavy damage on the ground. Each object has its own Impactor Table (IT) which shows many parameters useful to determine the risk assessment. As of September 2019, 551 of the risk-listed asteroids are considered too small (H > 25 and less than ~35 meters in diameter) to result in heavy damage on the ground. Ephemerides: It provides ephemerides of the object, that is position on sky, V magnitude, altitude, airmass, solar and lunar elongation, phase angle, galactic coordinates, R distance to the Sun, delta distance to the Earth, motion on sky, and the uncertainty on sky. Observation prediction: It provides the position of the object at a specific time, information useful for the observer and a graph showing the uncertainty on sky. Orbital Information: It provides the dynamical parameters of the orbit of the object. MOID: It shows the analysis of the Minimum Orbital Intersection Distance (MOID) of the object. Proper elements: It shows the secular properties of the object. Observational Information: It provides data of both optical and radar observations and their statistical performance. Close approaches: It provides a table with all the close approaches until 2100 with the planets of the Solar System. Search: It provides the possibility of queries in the database according to the orbital parameters or the observational conditions or the close approaches with the planets of the Solar System. Observatories: It is possible to access the information regarding observatories and their performances. Other services: Physical Information provided by ESA's NEO Coordination Centre; Orbit animation provided by the NEO Program Office at the Jet Propulsion Laboratory

How NEODyS works NEODyS is based on a Postgresql database running on a Linux system. The database of orbits is continually and automatically maintained with the most recent Minor Planet Center observations. The orbits are computed with the OrbFit software package provided by the OrbFit Consortium. All of the computational services provided by this site can also be done with this software package.

Future expansion of NEODyS NEODyS is continually expanding and improving. The following are the next tasks of the project:

Uncertainties of all the quantities provided with the orbit, e.g., MOID and absolute magnitude Variable time span for impact monitoring, based upon orbit uncertainty Inclusion of non-gravitational perturbations in the dynamic model

Major update On February 5, 2009 NEODyS went through a major update of the system. A new web-interface is available running the free software PHP. This allows a more flexible and easy to update system. In the same period the system switched to the new version of the Fortran 95 code OrbFit 4.0. Since 2011 NEODyS is operated and maintained for the European Space Agency by the University of Pisa spin-off SpaceDyS, based in Navacchio near Pisa. SpaceDyS provides data and scientific consultancy to the European Space Agency NEO Coordination Centre based in ESRIN, Frascati, Italy.

The NEODyS team The NEODyS team is composed by Fabrizio Bernardi (SpaceDyS, Italy), Andrea Chessa (SpaceDyS, Italy), Alessio Del Vigna (SpaceDyS, Italy), Linda Dimare (SpaceDyS, Italy), Davide Bracali Cioci (SpaceDyS, Italy), Giovanni F. Gronchi(University of Pisa, Italy), Giacomo Tommei (University of Pisa, Italy) and Giovanni B. Valsecchi (IASF-INAF, Rome, Italy). Pisa, Italy). The NEODyS founder was Andrea Milani (Dep. of mathematics, University of Pisa, Italy), Steve Chesley (Jet Propulsion Laboratory, USA) and María Eugenia San Saturio Lapeña (E.T.S. de Ingenieros Industriales, University of Valladolid, Spain).

See also List of near-Earth object observation projects

References

External links NeoDys official website Orbfit ESA NEO Coordination Centre

Worked examples

Example 1 — a first encounter with NEODyS

Start with the simplest possible case. Write down what NEODyS 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 NEODyS 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 NEODyS 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 NEODyS

In research
NEODyS 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 NEODyS 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
NEODyS is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical surveys, Near-Earth object tracking, so understanding it makes those chapters shorter.
In everyday life
Look for NEODyS 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 NEODyS in 20 minutes

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

Frequently asked questions

What is NEODyS in simple terms?

NEODyS (Near Earth Objects Dynamic Site) is an Italian service that provides information on near-Earth objects with a Web-based interface. It is based on a continually and (almost) automatically maintained database of near earth asteroid orbits.

Why does NEODyS 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 NEODyS?

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 NEODyS.

Tags

  • Astronomical surveys
  • Near-Earth object tracking

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