This celebrity’s a real star — or two

This celebrity’s a real star — or two

Hubble image of the Pistol Star • D. Figer (UCLA) and NASA

Originally published 27 October 1997

There is a new king of the hill.

The Hub­ble Space Tele­scope appears to have con­firmed the exis­tence of the most lumi­nous star ever observed, a gas-shroud­ed mon­ster near the cen­ter of the Milky Way Galaxy that is 10 mil­lion times brighter than the sun.

The star is buried in a cloud known as the Pis­tol Neb­u­la, for its shape. The star may have cre­at­ed the neb­u­la, by blow­ing off sheets of its own sub­stance. In any case, the “Pis­tol Star” makes good press, both for its name and because of our all-Amer­i­can fas­ci­na­tion with any­thing that qual­i­fies as biggest and most powerful.

How­ev­er, the press reports should car­ry a dis­claimer: “Not well understood.”

For one thing, the star is so far away, 25,000 light-years, and buried so deeply in its neb­u­la that it can­not be seen in vis­i­ble light. It was detect­ed only by the infrared radi­a­tion that it emits — radi­a­tion that pen­e­trates the clouds of gas that stand between us and the star.

Fur­ther­more, the image seen on the Hub­ble pho­to­graph may rep­re­sent the radi­a­tion of more than one star.

Final­ly, any­thing that hap­pens near the cen­ter of the galaxy is not as well under­stood as events in our own neigh­bor­hood, two-thirds of the way out towards the edge. The cen­ters of galax­ies are venues for lots of mys­te­ri­ous goings-on.

Still, the Pis­tol Star takes pos­ses­sion of our imag­i­na­tions. Here is a star, if it is a sin­gle star, that is born with tremors of vio­lence, blazes briefly as biggest and bright­est, and will die explo­sive­ly. In short, the Pis­tol Star is a celebri­ty among the tril­lion stars of the Milky Way Galaxy, and that alone attracts our atten­tion. It stretch­es our con­cep­tion of the possible.

Not so long ago the most lumi­nous known star was S Doradus, in the Large Mag­el­lan­ic Cloud, a small com­pan­ion galaxy of the Milky Way. S Doradus is a white-hot giant, near­ly a mil­lion times brighter than the Sun, but it too is “not well under­stood” and may not be a sin­gle star.

Among famil­iar stars, the bright­est are Deneb, the tail star of Cygnus the Swan, and Rigel, the for­ward foot of Ori­on. These stars are sure­ly what we make of them: sin­gle, hot super­giant stars, 60,000 times more lumi­nous than the sun. They are also 15 times clos­er than the Pis­tol Star.

Of “well under­stood” stars, Deneb and Rigel hold the hon­ors as kings of the hill.

And it is a hill. A cen­sus of stars accord­ing to their intrin­sic bright­ness (as opposed to their appar­ent bright­ness, which depends upon their dis­tance from us) would reveal a pyra­mid of types.

A look at the stars in our imme­di­ate neigh­bor­hood illus­trates the pattern.

With­in 20 light-years of Earth there are about 100 known stars. Of these, near­ly 70 are tiny red dwarf stars, much less bright than the sun, bare­ly hot enough to ignite the fires of nuclear fusion that blaze at a star’s core. These stars are so faint that they are not vis­i­ble to the naked eye, even though they are among our clos­est neighbors.

Our 20-light-year neigh­bor­hood includes about 15 orange stars, hot­ter and big­ger than the red dwarfs but not as hot or bright as the Sun.

There are six yel­low stars, includ­ing the Sun, with sur­face tem­per­a­tures of about 6,000 degrees Celsius.

Only three stars in the solar neigh­bor­hood are brighter than the sun: Pro­cy­on in Can­is Minor, Altair in Aquila the Eagle, and Sir­ius in Can­is Major. Sir­ius, a white-hot star, is the big boy on the block. The sun ranks 8th from the top of the pyramid.

A larg­er neigh­bor­hood, say 2,000 light-years in radius, would show the same pyra­mi­dal dis­tri­b­u­tion, but with a few blue-white super­giants sit­ting near the top, 2,000 times brighter than Sir­ius, includ­ing Deneb, Rigel and the stars of Ori­on’s belt.

Now, if the Hub­ble image has been inter­pret­ed cor­rect­ly, we have a new cap­stone for the galac­tic pyra­mid, big­ger and brighter than any star yet observed in the prime of its life.

The cap­stone stars pay a price for their dom­i­nance. They come and go quickly.

The red dwarfs at the bot­tom of the pyra­mid burn their hydro­gen fuel so slow­ly they live for hun­dreds of bil­lions of years. In fact, because the uni­verse is only about 15 bil­lion years old, every red dwarf star that was ever born is still with us.

Yel­low stars like the sun live for about 10 bil­lion years. Because the sun is less than 5 bil­lion years old, we have noth­ing to wor­ry about for anoth­er 5 bil­lion years.

But the biggest stars burn fast and vio­lent­ly. The Pis­tol Star, if it is a sin­gle star, is only a few mil­lion years old, and should blow itself to smithereens as a super­no­va with­in anoth­er few mil­lion years — a spec­tac­u­lar end to its brief reign as king of the hill.

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