Comfortable Materntiy Style Tips

You can be totally comfortable and cute during your pregnancy! Check out these tips to getting through your pregnancy in style and comfort.

woman shopping for clothes

Switch from heels to flats

Save your soles (and your ankles, calves and knees) by switching from high heels to small wedges or flat sandals or shoes, especially late in your pregnancy when you may be experiencing swelling in your extremities or loss of balance. Try cute ballet flats for the office and fun TOMS for running errands.

Remember that your feet may change during pregnancy. Measure your current size before doing any shoe shopping.

Rock a maxi dress

Whoever invented the maxi dress, we thank you! Maxi dresses are so comfortable, versatile and cute, you could wear one every day of your pregnancy. You may not even need a maternity style since the maxi dress’ flowy style has room for your growing bump. Choose one without any cinching at the waistline – opt instead for an empire waist.

Buy new lingerie

There is nothing worse than bra or undies cutting into your skin to make you feel reallllly uncomfortable. We highly suggest investing in some larger maternity/nursing bras and panties. Any amount of money spend on this endeavor is worth it, believe us!

Make sure the bra has extra support and wide, soft straps that won’t dig into your shoulders and that it fits snuggly (but not too tightly) around your body. Bras or panties should never leave behind red marks on your skin – that’s a sign that you need a larger size.

Ditch tight-fitting clothing

We’re not saying you can’t wear clothes that show off your pregnancy curves – we totally encourage proudly rocking your bump. However, even if you can fit into your non-maternity clothes for some time into your pregnancy, at some point you'll need to tuck your favorite skinny jeans into the back of your closet until after baby arrives and opt for some larger sizes, different styles or maternity clothes.

Opt for comfort and style with soft fabrics, like flowing tops paired with breathable leggings, stylish rompers and don’t forget that all important pregnancy piece, the maxi dress (we really can’t say this enough).

More on maternity clothes

The bare necessities: Building a maternity clothes survival kit

10 Ways to save on maternity clothes
Maternity wear: Do you really need it?


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The must-see pictures show in great detail the cratered surface of the tiny moon. Credit: NASA/JPL/Space Science InstituteDownload larger image version FIRST IMAGE: Phoebe's true nature is revealed in startling clarity in this mosaic of two images taken during Cassini's flyby on June 11, 2004. The image shows evidence for the emerging view that Phoebe may be an ice-rich body coated with a thin layer of dark material. Small bright craters in the image are probably fairly young features. This phenomenon has been observed on other icy satellites, such as Ganymede at Jupiter. When impactors slammed into the surface of Phoebe, the collisions excavated fresh, bright material -- probably ice -- underlying the surface layer. Further evidence for this can be seen on some crater walls where the darker material appears to have slid downwards, exposing more light-colored material. Some areas of the image that are particularly bright - especially near lower right - are over-exposed. An accurate determination of Phoebe's density - a forthcoming result from the flyby - will help Cassini mission scientists understand how much of the little moon is comprised of ices. This spectacular view was obtained at a phase, or Sun-Phoebe-spacecraft, angle of 84 degrees, and from a distance of approximately 32,500 kilometers (20,200 miles). The image scale is approximately 190 meters (624 feet) per pixel. No enhancement was performed on this image. Credit: NASA/JPL/Space Science InstituteDownload larger image version SECOND IMAGE: Phoebe delivers on its promise to reveal new wonders to Cassini by showing probable evidence of an ice-rich body overlain with a thin layer of dark material. The sharply-defined crater at above center exhibits two or more layers of alternating bright and dark material. Imaging scientists on the Cassini mission have hypothesized that the layering might occur during the crater formation, when ejecta thrown out from the crater buries the pre-existing surface that was itself covered by a relatively thin, dark lag deposit over an icy mantle. The lower thin dark layer on the crater wall appears to define the base of the ejecta blanket. The ejecta blanket itself appears to be mantled by a more recent dark surface lag.This image was obtained on June, 11 2004 at a phase, or Sun-Phoebe-spacecraft, angle of 79 degrees, and from a distance of 13,377 kilometers (8,314 miles). The image scale is approximately 80 meters (263 feet) per pixel. No enhancement was performed on this image. Credit: NASA/JPL/Space Science InstituteDownload larger image version THIRD IMAGE:This eye-popping high-resolution image of Phoebe's pitted surface taken very near closest approach shows a 13-kilometer (8-mile) diameter crater with a debris-covered floor. Part of another crater of similar size is visible at left, as is part of a larger crater at top and many scattered smaller craters. The radial streaks in the crater are due to downslope movements of loose fragments from impact ejecta. Also seen are boulders ranging from about 50 to 300 meters (160 to 990 feet) in diameter. The building-sized rocks may have been excavated by large impacts, perhaps from some other region of Phoebe rather than the craters seen here. There is no visible evidence for layering of ice and regolith or a hardened crust in this region, as on other parts of this moon. Some of the relatively bright spots are from small impacts that excavated bright material from beneath the dark surface. Images like this provide information about impact and regolith processes on Phoebe. This image was obtained at a phase, or Sun-Phoebe-spacecraft, angle of 78 degrees, and from a distance of 11,918 kilometers (7,407 miles). The image scale is approximately 18.5 meters (60.5 feet) per pixel. The illumination is from the right. 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An artist's concept shows the Cassini space probe at Saturn. Credit: NASA/JPLCassini's Ultraviolet Imaging Spectrograph (UVIS) detected the oxygen atoms spewing into a huge cloud on the dark side of Saturn's rings as Cassini prepared to enter orbit around Saturn in January 2004, said Donald Shemansky, professor of aerospace and mechanical engineering in the USC Viterbi School of Engineering. Data indicated that about 275 million pounds (125 million kilograms) of oxygen was abruptly released in a short period of time. "This was our first surprise in the ultraviolet," said Shemansky, who will analyze ultraviolet data during Cassini's four-year tour of Saturn and its rings with Janet Hallett, a postdoctoral aerospace research associate in the USC Viterbi School. "We aren't sure yet whether this was a transient event or part of a routine recycling process in Saturn's magnetosphere," he said. "Right now scientists are speculating that the oxygen eruption may have been caused by a collision of ice particles from the planet's distant E ring with material in one of the main ring systems, A, B or C. Or it could have been a meteorite collision or an eruption of icy slush on Enceladus, a moon that orbits in the E ring." Shemansky, a co-investigator on the 16-member Cassini ultraviolet imaging team, reported their findings in the Dec. 16 issue of Science Express . Despite Saturn's placid appearance from Earth, the planet is anything but that. The first detailed UV images from the Cassini mission show that Saturn commands a dynamic world of complex, braided ice rings, cannibalistic moons, 1,100 mile-per-hour planetary winds and electrifying auroral displays high in the night skies. Saturn, its moons and highly structured rings live inside a huge cavity in the solar wind created by the planet's strong magnetic field. The magnetosphere is a bubble of particles including electrons, various species of ions, neutral atoms and molecules, several populations of very energetic charged particles like those found in Earth's Van Allen Belts, and charged dust grains. The ionized (electrically charged) gases are called plasmas. However, unlike Jupiter's magnetosphere, Shemansky said Saturn's magnetic cocoon, which is smaller, is filled primarily with neutral gas rather than ions. "Saturn's magnetosphere is turning out to be very different from Jupiter's," he said. "It's dominated by neutral gas and water-rich ingredients produced by its rings, as icy moon debris collides, or by the more energetic collisions of incoming meteorites. It doesn't have nearly as many charged particles, and many of them are absorbed by the rings, so the plasma processes we are observing are entirely different." Two months after his initial observations, Shemansky and his ultraviolet team reported that the large cloud of escaping oxygen atoms had dissipated just as rapidly as it had appeared. Shemansky discounted theories that the rapid loss of material could be explained by "satellite sweeping," a process whereby tiny shepherding moons gobble up debris or deflect it as they clean out gaps between the rings. "The rate at which we saw material escaping from Saturn's outer rings implies that mass equivalent to the entire E ring, even including larger fragments and parent bodies, would be consumed in a period of about 100 million years if no replenishment processes are at work," he said. The rings of gas giants are made up of rocky debris from moons that have been torn apart by tidal waves or by an asteroid or comet collision during heavy bombardment periods. Rings are considered ephemeral and thought to disappear over time spans of billions of years. But Saturn's colorful rings appear to be younger than the planet itself, said scientists ? perhaps only 100 million years old, which is young in cosmological time. They also suspect that Saturn has had several ring systems in its history, although they have never had direct evidence on which to base their assumptions. "These observations are a first in solar system exploration," Shemansky said. "We have direct evidence now that the rings are made up of pure ice and that they are shaped by processes that happen fast," he added. "They aren't the same processes that shaped our solar system 4.5 billion years ago. "Given the fact that the outer rings are present at this time means that the system is being replenished by interactive plasma processes," Shemansky continued. "Clearly, the fact that something is eating up micron-sized grains in the outer ring zones at a high rate tells us that some sort of recycling process must be going on to rebuild them." Cassini's UV imaging spectrograph has made other significant observations. In the ultraviolet, scientists were able to see dust on the rings. Data showed variations in the amount of water-ice contained in the surfaces of ring particles, suggesting that darkened portions had been dusted with powder from pulverized moons or incoming meteoroids. The Cassini UVIS team also obtained ultraviolet images of Phoebe, Saturn's most distant large moon, during the inbound flight to Saturn. Data showed the absorption lines of water-ice on Phoebe's dark surface, which gave scientists more clues about its origins. The only moon in the Saturnian system to orbit in a retrograde, or backward, direction, Phoebe is similar to a common C-type carbonaceous asteroid. Scientists theorize that it was flung out of the Kuiper Belt, a region well beyond Neptune's orbit where thousands of small, icy comets reside, and sucked up by Saturn's strong gravitational field, but no one is absolutely sure of its origin. 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