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This sounds like a no-brainer, but many times a couch, chair, or bed moved during the summer stays there in winter, blocking the flow of heat into the room. This wastes money and leads to cold rooms. With a forced-air system, blocking a supply or return vent can cause a house-wide pressure imbalance that disrupts the heat flow in the whole system.
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If you feel cold air seeping beneath a door leading outside and find that using a door snake is inconvenient (see item #6), install a draft-defeating nylon door sweep. This long, thin broom-like vinyl-and-pile attachment gets installed along the inside bottom edge of the door. Cut the sweep to fit with a hacksaw and keep it in place with four or five wood screws.
If you have a forced-air system, changing the furnace filter can save you some energy (up to 5 percent) and keep dust down in the house. The system will last longer and be less likely to break down. The most popular 16 X 20-inch duct filter costs around 50 cents when bought by the box. Change them monthly during heating season. Measure your air filter before shopping; they range in size from 12 X 12 inches to 30 X 30 inches. An alternative to swapping out the replacement filter is to use washable filters (around $20 each). With care, they can last five years.
It might surprise you to learn, however, that these parameters are all interrelated. For example, we might have the expansion rate wrong; it might be more like 73 km/s/Mpc, as favored by groups who use late-time, distance ladder measurements (like supernovae) as opposed to the 67 km/s/Mpc obtained by early-time, relic signal methods (like the cosmic microwave background and baryon acoustic oscillations). That would change the expansion rate, today, by about 9% from the preferred value.
Globular clusters exist in every large galaxy; some contains hundreds (like our Milky Way), others, like M87, can contain more than 10,000. Each globular cluster is a collection of many stars, ranging from a few tens of thousands up to many millions, and each star within it will have a color and a luminosity: both easily measurable properties. When we plot the color and magnitude of each star within a globular cluster together, we get a particularly shaped curve that snakes from the lower-right (red color and low luminosity) to the upper-left (blue color and high luminosity).
After the Big Bang, the universe was like a hot soup of particles (i.e. protons, neutrons, and electrons). When the universe started cooling, the protons and neutrons began combining into ionized atoms of hydrogen (and eventually some helium). These ionized atoms of hydrogen and helium attracted electrons, turning them into neutral atoms - which allowed light to travel freely for the first time, since this light was no longer scattering off free electrons. The universe was no longer opaque! However, it would still be some time (perhaps up to a few hundred million years post-Big Bang!) before the first sources of light would start to form, ending the cosmic dark ages. Exactly what the universe's first light (ie. stars that fused the existing hydrogen atoms into more helium) looked like, and exactly when these first stars formed is not known. These are some of the questions Webb was designed to help us to answer. See also our Q&A with John Mather about the Big Bang.
After the Big Bang, the universe was like a hot soup of particles (i.e. protons, neutrons, and electrons). When the universe started cooling, the protons and neutrons began combining into ionized atoms of hydrogen and deuterium. Deuterium further fused into helium-4. These ionized atoms of hydrogen and helium attracted electrons turning them into neutral atoms. Ultimately the composition of the universe at this point was 3 times more hydrogen than helium with just trace amounts of other light elements.
This process of particles pairing up is called "Recombination" and it occurred approximately 240,000 to 300,000 years after the Big Bang. The Universe went from being opaque to transparent at this point. Light had formerly been stopped from traveling freely because it would frequently scatter off the free electrons. Now that the free electrons were bound to protons, light was no longer being impeded. "The era of recombination" is the earliest point in our cosmic history to which we can look back with any form of light. This is what we see as the Cosmic Microwave Background today with satellites like the Cosmic Microwave Background Explorer (COBE) and the Wilkinson Microwave Anisotropy Probe (WMAP). Following this are the cosmic dark ages - a period of time after the Universe became transparent but before the first stars formed. When the first stars formed, it ended the dark ages, and started the next epoch in our universe.
Every entree at The Old Spaghetti Factory is served with hot fresh baked bread, soup or crisp green salad, and a scoop of our signature spumoni or vanilla ice cream. Our menu is full of flavorful value that feels just like home.
From our vantage point on Earth, the Sun may appear like an unchanging source of light and heat in the sky. But the Sun is a dynamic star, constantly changing and sending energy out into space. The science of studying the Sun and its influence throughout the solar system is called heliophysics.
Visible light from these top regions of the Sun is usually too weak to be seen against the brighter photosphere, but during total solar eclipses, when the Moon covers the photosphere, the chromosphere looks like a fine, red rim around the Sun, while the corona forms a beautiful white crown ("corona" means crown in Latin and Spanish) with plasma streamers narrowing outward, forming shapes that look like flower petals.
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Begonia 'Santa Cruz Sunset' (Begonia boliviensis). 'Santa Cruz Sunset' packs both flower power and bold color. It boasts a compact, upright habit during its early stages of growth, but as it matures, plants begin to cascade over edges of pots and baskets. Fiery bright red-orange, bell shaped flowers cover the entire plant, creating a lush tropical look. At maturity it averages 12-16" in height and spreads 16-20".
Corn, Ornamental 'Japonica Striped Maize' (Zea spp.). A beautiful ornamental pop corn from Japan, 'Japonica Striped Maize' grows 5-6 feet tall and boasts variegated leaves striped with green, white, yellow and pink. It produces dark purple tassels and burgundy kernels or corn. Color development is better when plants are widely spaced. As an added bonus, the mature ears are sought-after by birds.
Zinnia 'Profusion Double Hot Cherry' (Zinnia hybrida). 2013 AAS Winner. This new zinnia was recognized by AAS judges for holding its vibrant cherry red color throughout the season. It displays a compact growth habit and good disease resistance. A highly prolific bloomer, 'Profusion Double Hot Cherry' produces masses of 2" double flowers on mid-height plants. It performs exceptionally well in gardens, planters and landscapes, due to is combined tolerance for both cool and hot, humid conditions. Plants mature 12-18" in height with a 16-24" spread.
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The Bossa Nova Civic Club New York at Bushwick is billed as a "tropical fantasy dance club". That description is pretty much spot on, and we guarantee that you won't see another place quite just like it. Underground house and techno are the order of the day here, and the sound system is absolutely pounding. There is always a steady stream of high profile DJs manning the turntables here, so get ready for a night that you won't soon forget.
Located on the site of what was formerly Club Europa, the Good Room at Greenpoint perfectly displays the extensive redesign work done by nightlife guru Steve Lewis. Since the club was opened in 2014, it has taken its place among the top nightspots in the city. The drinks are pretty reasonably priced, which is always a pleasant surprise, and the sound system is as booming as they come. If you and your New York escort don't feel like braving your way through yet another glitzy Brooklyn's nightspot, the Good Room is the perfect alternative. 041b061a72