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TiliK225 [7]
3 years ago
5

Gizmo force and fan cart

Physics
1 answer:
liberstina [14]3 years ago
8 0

Answer:

see I need help for chemistry pls anyone here helps me I must submit before 10:30

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Black holes are highly condensed remnants of stars. Some black holes, together with a normal star, form binary systems. In such
borishaifa [10]

\lambda_\text{max} = 2.63\times 10^{-9}\;\text{m}.

<h3>Explanation</h3>

The peak emission wavelength of an object depends on its absolute temperature.

\lambda_\text{max} = \dfrac{2.90\times 10^{-3}}{T},

where

  • \lambda_\text{max} is the wavelength in meters where the emission is the strongest.
  • T is the temperature of the object in degrees Kelvins.

For the gas falling into the black hole,

T = 1.10\times 10^{6}\;\text{K}.

Apply the formula:

\lambda_\text{max} = \dfrac{2.90\times 10^{-3}}{T} = \dfrac{2.90\times 10^{-3}}{1.10\times 10^{6}} = 2.64\times 10^{-9}\;\text{m} = 2.64 \;\text{nm}.

The question mentioned that \lambda_\text{max} is in the X-ray region of the electromagnetic spectrum. According to Encyclopedia Britannica, the wavelength of X-rays range from 10^{-8}\;\text{m}=10\;\text{nm} to 10^{-10}\;\text{m} = 0.1\;\text{nm}, which indeed includes 2.64\times 10^{-9}\;\text{m} = 2.64 \;\text{nm}.

4 0
3 years ago
Plzzz help me fast i have absolutly no f-r-i-c-k-e-n idea what this is or how to do it
vodomira [7]

P.E =mgh

=5o x 4 x 10

Explanation:

= 2000J

4 0
3 years ago
Read 2 more answers
The sun has sufficient hydrogen to continue fusing into helium for how much longer?
vichka [17]

Answer:

4500 million years

Explanation:

The Sun shines thanks to the thermonuclear conversion of hydrogen to helium inside. It is currently 4,500 million years old and has reservations for a similar period of time. When this fuel is exhausted in the central region, the heart of the Sun, constituted of helium and in an inert state, will contract and put more external fuel reserves within reach of the star, with which this mass of helium will grow over time . When that happens, the Sun will evolve into a giant star that will reach the orbit of Mars and, therefore, destroy the planet Earth.

As the helium heart mass increases so do the central density and temperature. When it reaches 100 million degrees, helium fuses thermonuclearly with itself and becomes a mixture of carbon and oxygen.

When the helium runs out in the center, the previous operation is reproduced approximately. The carbon / oxygen heart contracts and the helium and hydrogen of the surrounding layers are placed within the reach of thermonuclear combustion. The difference is that this double combustion is unstable and the density is so high that electrons can, alone, stabilize the heart of carbon and oxygen. The end result is that the outer layers, which originate a planetary nebula, are expelled, and the old thermonuclear reactor becomes visible, which becomes a white dwarf that slowly cools like the embers of a fire over billions of millions. of years.

8 0
3 years ago
What do we mean by the event horizon of a black hole?
Evgen [1.6K]

It is the point in a black hole where nothing, not even light, can escape from.

8 0
4 years ago
How many total atoms are in 2CuSO4 A.2 B.6 C.8 D.12​
makvit [3.9K]

That depends on how much of it you have, but it's a hugely enormous gigantic number in even the smallest sample.

You can see from the formula that there are 12 atoms in every molecule of the stuff !

5 0
3 years ago
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