Warm

1. Also, your affected leg may feel warm and be redder than the other leg.
2. Also, the leg may feel warm and look redder than the other leg.

Pluto

1. Pluto has become significantly redder, while its illuminated northern hemisphere is getting brighter. (Web site)

Darker

1. From the ragged edge of the polar cap northward, the satellite's face is generally darker and redder in color. (Web site)

Skin Rash

1. A clue to these forms of allergy would be if the skin rash becomes worse (redder and more itchy) rather than better after applying a cream or ointment. (Web site)

Base Metal

1. Copper is the most commonly used base metal, yielding a redder color. (Web site)
2. Copper is the most commonly used base metal, yielding a redder metal. (Web site)

Sun

1. B-V is zero for the star Vega (spectral class A0), and is about 0.61 for the Sun which is redder than Vega.

Massive

1. The stars in globular clusters are generally older, redder and less massive than our Sun. (Web site)

Nucleus

1. The nucleus appears more yellow thanthe spiral arms as it contains a higher proportionof dust and older, redder stars.

Billion Years

1. Two photons produced by a gamma-ray burst 10 billion years ago, one redder and one bluer, should arrive on Earth at slightly different times. (Web site)

Light

1. When an object is traveling away from the Earth The light from this object is stretched out, making it look redder. (Web site)

Brighter

1. The bright nucleus of M101 just off to the upper left appears brighter and redder than the rest of the galaxy seen in the image. (Web site)

Star Clusters

1. Once formed, the star clusters become redder with age as the most massive and bluest stars exhaust their fuel and burn out. (Web site)

Galaxies

1. For instance, elliptical E galaxies appear redder than S galaxies, which indicates that they consist of older, redder stars and stellar clusters. (Web site)

Bright Blue

1. On the outside is a ring dominated by bright blue stars, while near the center lies a ball of much redder stars that are likely much older. (Web site)

Wavelengths

1. The light from galaxies at much larger distances is stretched to longer, redder wavelengths ["redshifted"], due to the expansion of the universe.
2. This movement shifts the light toward the red end of the spectrum because the light waves are stretched to longer (redder) wavelengths. (Web site)

Visible Spectrum

1. Here, the term "redder" refers to what happens when visible light is shifted toward the red end of the visible spectrum. (Web site)

Cooler

1. Cooler stars emit more light at longer wavelengths (and so appear redder than hot stars). (Web site)
2. Both stars are only about a third the mass of our sun and are much cooler and redder in color. (Web site)
3. The star cluster will continue its evolution with the smaller, hence cooler and redder, stars. (Web site)

Older

1. Stars in the bulge of the our own Milky Way Galaxy are also typically older and redder than stars in the disk where our Sun resides.
2. The disk is nested inside an elliptical ring of older, cooler, redder stars, which was seen in previous Hubble observations. (Web site)
3. In contrast to the blue disk, the bright central bulge is made up of mostly older, redder stars. (Web site)

Central Bulge

1. The central bulge stars are older and redder than disk stars, which appear more blue.

Redder

1. Spiral galaxies contain a larger number of bluer, younger stars, while elliptical galaxies contain a larger number of redder, older stars. (Web site)
2. Redder (longer wavelength) light is scattered less by atmosphere molecules and dust than bluer (shorter wavelength) light. (Web site)
3. Most stars in globular clusters are older and redder than our Sun, which is about 5 billion years old. (Web site)

Categories

1. Central Bulge
2. Elliptical Galaxies
3. Older
4. Bright Nucleus
5. Cooler
6. Books about "Redder" in Amazon.com
   

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