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The origins of the strong magnetic field are as yet unclear.

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Likewise, a collapsing star begins with a much larger surface area than the resulting neutron star, and conservation of magnetic flux would result in a far stronger magnetic field. However, this simple explanation does not fully explain magnetic field strengths of neutron stars. The energy comes from the gravitational binding energy of a neutron star. Hence, the gravitational force of a typical neutron star is huge. If an object were to fall from a height of one meter on a neutron star 12 kilometers in radius, it would reach the ground at around kilometers per second.

Because of the enormous gravity, time dilation between a neutron star and Earth is significant. For example, eight years could pass on the surface of a neutron star, yet ten years would have passed on Earth, not including the time-dilation effect of its very rapid rotation. Neutron star relativistic equations of state describe the relation of radius vs.

BE is the ratio of gravitational binding energy mass equivalent to the observed neutron star gravitational mass of "M" kilograms with radius "R" meters, [40]. Its mass fraction gravitational binding energy would then be 0. This is not near 0.

The equation of state for a neutron star is not yet known. It is assumed that it differs significantly from that of a white dwarf, whose equation of state is that of a degenerate gas that can be described in close agreement with special relativity. However, with a neutron star the increased effects of general relativity can no longer be ignored. For example, a 1. Current understanding of the structure of neutron stars is defined by existing mathematical models, but it might be possible to infer some details through studies of neutron-star oscillations.


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Asteroseismology , a study applied to ordinary stars, can reveal the inner structure of neutron stars by analyzing observed spectra of stellar oscillations. Current models indicate that matter at the surface of a neutron star is composed of ordinary atomic nuclei crushed into a solid lattice with a sea of electrons flowing through the gaps between them.

It is possible that the nuclei at the surface are iron , due to iron's high binding energy per nucleon. The "atmosphere" of a neutron star is hypothesized to be at most several micrometers thick, and its dynamics are fully controlled by the neutron star's magnetic field. Below the atmosphere one encounters a solid "crust". Proceeding inward, one encounters nuclei with ever-increasing numbers of neutrons; such nuclei would decay quickly on Earth, but are kept stable by tremendous pressures. As this process continues at increasing depths, the neutron drip becomes overwhelming, and the concentration of free neutrons increases rapidly.

In that region, there are nuclei, free electrons, and free neutrons. The nuclei become increasingly small gravity and pressure overwhelming the strong force until the core is reached, by definition the point where mostly neutrons exist. The expected hierarchy of phases of nuclear matter in the inner crust has been characterized as " nuclear pasta ", with fewer voids and larger structures towards higher pressures.

One model describes the core as superfluid neutron-degenerate matter mostly neutrons, with some protons and electrons. More exotic forms of matter are possible, including degenerate strange matter containing strange quarks in addition to up and down quarks , matter containing high-energy pions and kaons in addition to neutrons, [10] or ultra-dense quark-degenerate matter. Neutron stars are detected from their electromagnetic radiation.

Neutron stars are usually observed to pulse radio waves and other electromagnetic radiation, and neutron stars observed with pulses are called pulsars. Pulsars' radiation is thought to be caused by particle acceleration near their magnetic poles , which need not be aligned with the rotational axis of the neutron star. It is thought that a large electrostatic field builds up near the magnetic poles, leading to electron emission. The radiation emanating from the magnetic poles of neutron stars can be described as magnetospheric radiation , in reference to the magnetosphere of the neutron star.

If the axis of rotation of the neutron star is different to the magnetic axis, external viewers will only see these beams of radiation whenever the magnetic axis point towards them during the neutron star rotation. Therefore, periodic pulses are observed, at the same rate as the rotation of the neutron star.

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In addition to pulsars, neutron stars have also been identified with no apparent periodicity of their radiation. In addition to radio emissions, neutron stars have also been identified in other parts of the electromagnetic spectrum. This includes visible light , near infrared , ultraviolet , X-rays and gamma rays. The majority of neutron stars detected, including those identified in optical, X-ray and gamma rays, also emit radio waves; [50] the Crab Pulsar produces electromagnetic emissions across the spectrum.

Neutron stars rotate extremely rapidly after their formation due to the conservation of angular momentum; like spinning ice skaters pulling in their arms, the slow rotation of the original star's core speeds up as it shrinks. A newborn neutron star can rotate many times a second. Over time, neutron stars slow, as their rotating magnetic fields in effect radiate energy associated with the rotation; older neutron stars may take several seconds for each revolution. This is called spin down. The rate at which a neutron star slows its rotation is usually constant and very small.

The periodic time P is the rotational period , the time for one rotation of a neutron star. However, as a neutron star ages, the neutron star slows P increases and the rate of slowing decreases P -dot decreases. Eventually, the rate of rotation becomes too slow to power the radio-emission mechanism, and the neutron star can no longer be detected.

P and P -dot allow minimum magnetic fields of neutron stars to be estimated. It is not the measured luminosity, but rather the calculated loss rate of rotational energy that would manifest itself as radiation. For neutron stars where the spin-down luminosity is comparable to the actual luminosity , the neutron stars are said to be " rotation powered ".

P and P -dot can also be plotted for neutron stars to create a P — P -dot diagram. It encodes a tremendous amount of information about the pulsar population and its properties, and has been likened to the Hertzsprung—Russell diagram in its importance for neutron stars. Neutron star rotational speeds can increase, a process known as spin up. Sometimes neutron stars absorb orbiting matter from companion stars, increasing the rotation rate and reshaping the neutron star into an oblate spheroid.

This causes an increase in the rate of rotation of the neutron star of over a hundred times per second in the case of millisecond pulsars. The most rapidly rotating neutron star currently known, PSR Jad , rotates at revolutions per second. However, at present, this signal has only been seen once, and should be regarded as tentative until confirmed in another burst from that star. Sometimes a neutron star will undergo a glitch , a sudden small increase of its rotational speed or spin up.

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Glitches are thought to be the effect of a starquake —as the rotation of the neutron star slows, its shape becomes more spherical. Due to the stiffness of the "neutron" crust, this happens as discrete events when the crust ruptures, creating a starquake similar to earthquakes. The Advanced Atlas Test. Here are some cities that are particularly good for testing whether your atlas is completely trustworthy. Even atlases that generally do well may fail at some of these.

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When software authors choose to develop their own atlases, instead of using the industry-standard ACS atlas data, errors can creep it and places omitted. At the time of testing, December , several major programs couldn't find a city or gave the wrong time zone for a place or two, but I'm happy to report that every manufacturer immediately addressed the issue.

Please remember to get the latest atlas updates when they become available for your software. Important Note : If you are creating charts for newborns living in foreign countries, go to www. According to David Cochrane of Cosmic Patterns, this website is an excellent source for accurate contemporary time zone information.


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  8. For example, Venezuela has changed the time zone used countrywide. Thanks to David Cochrane for this alert. Unfortunately, the ACS atlas has not been updated to reflect this change, and so programs that rely on it -- such as Solar Fire, TimePassages, Shri Jyoti Star -- will create incorrect charts for Venezuela for newborns until this issue has been addressed. Even versions of Kepler or Sirius that have not been recently updated will have this problem. So for recent births outside of the U.

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    To test whether your program can calculate time zones correctly: You can use 12 noon i. Limitations in software design: A. Missed Events. A longstanding problem that existed in earlier versions of many astrology programs -- and still exists in one current program -- is that if you rely on your astrology software to search for outer planet transits and you limit the search to only a couple of months, they left out very major events.

    Note: The Time Line graphical transit display in Kepler and Sirius does not have this problem, and it is possible to configure their hit listings to avoid this too by going to Dates and Times to Print, and changing "the number of months before and after printout to find: aspects in orb" to two months. They find events that have already entered orb but have not reached an exact hit. The problem is the result of the fact that Uranus, Neptune, and Pluto slow down and change direction twice a year, and near each station, they may approach an exact aspect for several months.

    If the beginning date of the transit search happens to be after the transiting planet has entered a one degree orb, and for the duration of the search the transiting planet never exactly aspects the natal planet, then the software will not list the event at all! Here's an example: Bill Clinton was in a period of Neptune opposed Saturn during September and October of , but almost every astrology program completely omitted this transit if the search period was from September 1, thru November 15, because at the starting date the transit has passed the entering orb, and it didn't reach the exact hit until November 27, In the above image, we can see that Neptune entered one degree orb on July 20 and reached exactness on August But in October, Neptune stationed, and so Neptune doesn't exactly oppose Saturn again until November 27th.

    If an astrologer searches for major transits during September and October for Bill Clinton using most astrology programs, the transit will not show up. Feel free to test your software using the above example. Bill Clinton's birth data is: August 19 , am, Hope, Arkansas.

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    This very serious deficiency in most astrology programs and can only be compensated for by setting your software to look for periods of at least three months at a time if you are using a one degree approaching orb. If you are an astrologer who uses much wider transit orbs, like 6 degrees, your software becomes won't find many major transits unless you do scans of two years or more.

    Missed Events in Kepler and Sirius Hit Lists : The transit text listings in both Kepler and Sirius will omit some stationary events for short transit scans, but you can fix this if you make one small change in them. After running a transit listing, you right-click and customize the report: changing the Aspects in Orb to 1 instead of 0. Stations within Orb. Most astrology programs can list planetary stations, but not in relationship to specific transits. Since, often, the most powerful transits are ones where the transiting planet approaches a natal point and then stands still nearby before reaching an exact hit, this omission is significant.