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What stars are called new? Detailed answer

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What stars are called new?

Each year, 25-30 (by some estimates, even more than 200) new stars flare up in the Galaxy, although only a few of them are observed. The novae are characterized by an extremely rapid increase in brightness by thousands and even millions of times (by an average of 12 magnitudes, that is, 60 thousand times) over several days and a subsequent slow return to the initial state over several months or years (first, the brightness of the star faster and then it slows down).

A nova is a binary star, one component of which is a white dwarf and the other is either a star like the Sun or a red giant. The period of revolution of the components of this binary star is only a few hours, and therefore, the distance between them is quite small and the interaction forces are quite large.

When the second component of such a binary star expands in the course of its evolution, passing a certain boundary (the so-called Roche limit), part of its matter flows into the white dwarf. At the same time, such temperature and pressure are created on the surface of the white dwarf that the nuclear reaction becomes explosive, which explains the sharp increase in the brightness of the star.

Expanded (bloated) hundreds of thousands of times, the star separates at the moment of maximum brightness a gaseous shell, equal in mass to 0,00001-0,0001 of the mass of the Sun. That, gradually expanding, dissipates in space. The expansion rate of nova shells is about 1000 kilometers per second.

A distinctive feature of many new stars is the recurrence of their outbursts. The intervals between outbursts in repeated novae range from several tens to several thousand years (they are longer for those repeated novae that increase brightness more strongly).

Outwardly, the new ones are similar to supernovae, although in general we are talking about completely different phenomena and the energy released during the explosion is less than a million times.

Author: Kondrashov A.P.

 Random interesting fact from the Great Encyclopedia:

What are elements?

All matter is made up of elements. Elements are substances made up of atoms of only one kind. Many elements have similarities with each other, sometimes even very significant, but among them no two are absolutely identical. For example, hydrogen and helium are both colorless, odorless, and tasteless gases. However, hydrogen is lighter than helium. It burns in the presence of oxygen, but helium does not.

Elements differ from each other by atomic weight. Some of them under normal conditions are solids, others are liquids, and still others are gases. When heated or cooled, many of them (almost all) can go from one state to another. Some elements dissolve in water, others do not. These and many other characteristics of elements are called their physical properties. Elements can interact with each other (with a few exceptions), forming various substances. Such interactions are called chemical reactions. The ability of an element to enter into a particular reaction is determined by its chemical properties.

In accordance with their physical and chemical properties, all elements are divided into several groups. They include elements with similar properties. These groups together make up the periodic table of elements of D. I. Mendeleev. It is named after the Russian chemist Dmitri Ivanovich Mendeleev, who came up with the idea of ​​creating this table.

 The order of arrangement of elements in the table of D. I. Mendeleev is determined by their serial atomic number. The serial number of an element depends on the number of protons - positively charged particles - in the nucleus of an atom of a given element. The hydrogen atom contains only one proton and therefore occupies the first place in the periodic table. Some elements were named after great scientists, such as einsteinium (Einstein). Others are in honor of countries or certain areas on the globe: germanium (Germany), ruthenium (Russia), california (California), scandium (Scandinavia). Still others are named for their special properties: indium (because of its bright indigo blue color). Many elements are well known to everyone: copper, iron, lead, silver, gold, aluminum, sulfur, mercury, iodine and many others.

 Test your knowledge! Did you know...

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Accelerometer ST Microelectronics LIS3DHH 26.07.2017

The new accelerometer LIS3DHH was created specifically for use in inclinometers - devices for accurately measuring the angles of an object. To ensure exceptionally high accuracy performance, the LIS3DHH has only one measuring range of ±2.5 g. The relatively large 5mm x 5mm ceramic case serves the same purpose.

The new chip features a low noise level of 45 ?g/vHz and excellent temperature and time stability (<0.4 mg/°C). It is suitable for use in test equipment, for stabilizing antenna platforms and in measuring instruments.

The zero shift for LIS3DHH does not exceed ±60 mg. The microcircuit has an uncalibrated temperature sensor with a resolution of 16 units / degree and a noise of 0.1 ° C (RMS). The operating voltage of LIS3DHH is 1,71 ... 3,6 V, and the current consumption is 2,5 mA.

Features LIS3DHH:

3-axis, ±2.5 g full scale
Ultra-low noise: 5µg/vHz
Excellent temperature stability: <0.4 mg/°C
Output data 16-bit
SPI 4-wire digital interface
Temperature sensor output 12 bit
Embedded FIFO (32 levels deep)
High overload resistance
Temperature -40 °C ... +85 °C

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