SOLAR NEWS:
March 9,2015 | {M5.8 M4.5 C9.1}
Class Solar-Flares_Triple
Blackout!
Sirius A & B:
http://en.wikipedia.org/wiki/Sirius
An artist's impression of Sirius A and
Sirius B. Sirius A is the larger of the two stars.
§Sirius A has a mass of 2 M☉. The radius of this star has been measured by an astronomical interferometer, giving an estimated angular diameter of 5.
936±0.
016 mas. The projected rotational velocity is a relatively low 16 km/s, which does not produce any significant flattening of its disk. This is at marked variance with the similar-sized
Vega, which rotates at a much faster 274 km/s and bulges prominently around its equator. A weak magnetic field has been detected on the surface of Sirius A.
Stellar models suggest that the star formed during the collapsing of a molecular cloud, and that after
10 million years, its internal energy generation was derived entirely from nuclear reactions.
The core became convective and utilized the
CNO cycle for energy generation. It is predicted that Sirius A will have completely exhausted the store of hydrogen at its core within a billion years of its formation. At this
point it will pass through a red giant stage, then settle down to become a white dwarf.
Sirius A is classed as an Am star because the spectrum shows deep metallic absorption lines, indicating an enhancement in elements heavier than helium, such as iron. When compared to the Sun, the proportion of iron in the atmosphere of Sirius A relative to hydrogen is given by \begin{smallmatrix}[\frac{Fe}{
H}]=0.5\end{smallmatrix}, which is equivalent to
100.5, meaning it has 316% of the proportion of iron in the Sun's atmosphere. The high surface content of metallic elements is unlikely to be true of the entire star, rather the iron-peak and heavy metals are radiatively levitated towards the surface.
§Sirius B
The orbit of Sirius B around A as seen from
Earth (slanted ellipse). The wide horizontal ellipse shows the true shape of the orbit (with an arbitrary orientation) as it would appear if viewed straight on.
With a mass nearly equal to the Sun's, Sirius B is one of the more massive white dwarfs known (0.98 M☉); it is almost double the 0.5–0.6 M☉ average. Yet that same mass is packed into a volume roughly equal to the Earth's. The current surface temperature is 25,
200 K. However, because there is no internal heat source, Sirius B will steadily cool as the remaining heat is radiated into space over a period of more than two billion years.
A white dwarf forms only after the star has evolved from the main sequence and then passed through a red-giant stage. This occurred when Sirius B was less than half its current age, around
120 million years ago. The original star had an estimated 5 M☉ and was a
B-type star when it still was on the main sequence. While it passed through the red giant stage, Sirius B may have enriched the metallicity of its companion.
This star is primarily composed of a carbon–oxygen mixture that was generated by helium fusion in the progenitor star. This is overlaid by an envelope of lighter elements, with the materials segregated by mass because of the high surface gravity. Hence the outer atmosphere of Sirius B is now almost pure hydrogen—the element with the lowest mass—and no other elements are seen in its spectrum.
§Sirius star cluster
In
1909,
Ejnar Hertzsprung was the first to suggest that Sirius was a member of the
Ursa Major Moving Group, based on his observations of the system's movements across the sky. The
Ursa Major Group is a set of
220 stars that share a common motion through space and were once formed as members of an open cluster, which has since become gravitationally unbound. However, analyses in
2003 and
2005 found Sirius's membership in the group to be questionable: the Ursa Major Group has an estimated age of
500±
100 million years, whereas Sirius, with metallicity similar to the Sun's, has an age that is only half this, making it too young to belong to the group. Sirius may instead be a member of the proposed Sirius
Supercluster, along with other scattered stars such as
Beta Aurigae,
Alpha Coronae Borealis,
Beta Crateris,
Beta Eridani and
Beta Serpentis. This is one of three large clusters located within 500 light-years (
150 pc) of the Sun.
The other two are the
Hyades and the
Pleiades, and each of these clusters consists of hundreds of stars.
SDO: http://sdo.gsfc.nasa.gov/
Helio: http://helioviewer.org/
ISWA: http://iswa.ccmc.gsfc.nasa.gov/IswaSystemWebApp/
SWPC: http://www.swpc.noaa.gov/
Spaceweather: http://www.spaceweather.com/
- published: 10 Mar 2015
- views: 140