Dimensions: 27 x 15 x 69 cm Colour black with silver prints Handle to hold the backpack in hand Fastening strap around the waist Back of the backpack with an insert with a soft sponge lined with mesh to secure the lumbar region The opening and closing from the top with a velcro The outer zippered pocket Possible connection of the upper and lower part of the backpack Click here to download full size table for SANTI products Click here to download the drysuit manual Click here to download the Heating System Manual Click here to download ™SANTI CatalogueThe only time you may not fully enjoy the vistas of Sedona’s red rocks is when they’re growing smaller in your rearview mirror. It’s always hard to say goodbye to a Sedona vacation. You want to linger a little longer on the trail, watch one more sunset or browse in one more shop. When you do finally have to head home, take more than just amazing memories with you. As meaningful as the memories are to you and your family, you can’t mount them on your wall, hang them in your closet or gift wrap them for a friend’s birthday.

As one of the Southwest’s premier arts communities, Sedona is a paradise for collectors and buyers. Galleries feature traditional Western, contemporary Southwestern and Native American art. You’ll also find wearable art, home décor, garden accents, outdoor gear, books, music, gift items, souvenirs and so much more. Several New Age shops specialize in items for those on a personal journey, such as crystals, candles and aromatherapy oils.tusting backpack Don’t look for malls or charmless big box stores. ataka backpackSedona’s shopping areas are woven into the fabric of the town. gypsy backpack typoAnd like everything else, very connected to the dazzling scenery. hcsc backpack

Shopping is one more outdoor activity in Sedona. You just carry bags instead of backpacks and have more footwear options. Roam the streets, prowl the plazas and every time you step out of a store the soaring red rocks are there to greet you, like old friends eager to share in your newly purchased treasures. You’ll find shopping throughout Sedona but here’s a simple guide to help get you started.backpack h1z1 crafting Uptown Sedona, at the intersection of Arizona 89A and 179, is packed with galleries, gift shops, cafes and restaurants. thule backpack 21lCompact and easily walked, Uptown serves as the central hub of Sedona. An eclectic assortment of retail businesses are tucked into every nook and cranny and it’s hard to proceed more than a few steps before some eye-catching jewelry or sculpture, or just-right T-shirt pulls you in off the sidewalk.

Perched on a hill overlooking Uptown, the Shops at Hyatt Piñon Pointe include upscale galleries, clothing stores and eateries. To the south, nestled on the banks of Oak Creek, sits Tlaquepaque Arts and Crafts Village, a collection of Spanish-style buildings reminiscent of a Mexican hamlet. Cobblestone walkways, splashing fountains and giant, graceful Arizona sycamores that seem to grow from the buildings themselves make this an unforgettable destination. Soak up the sights but don’t forget about the myriad galleries and shops tucked beneath arched doorways. The Arizona 179 corridor, often called the Gallery District, is lined with restaurants and world-class galleries, clustered in small plazas, such as Hozho Center and Hillside Sedona. This stretch includes such notable landmarks as the Chapel of the Holy Cross and Cathedral Rock. Arizona Highway 179 has been declared a Red Rock Scenic Byway, and dishes up dramatic and far-reaching views. The Village of Oak Creek, further south along 179, and West Sedona, along 89A, are more traditional shopping and service areas but also bristling with opportunities to find artwork and products unique to Sedona.

CategoryEquipment > Vehicle Parts Sedan Wheel is a vehicle repair component in DayZ Standalone. It is one of several parts necessary to get a Sedan in running order. The Sedan Wheel can be repaired by Duct Tape. Dual side adjustment straps for the perfect fit; open sides provide freedom of movement, ventilation and improved comfortcomfortable 3D front panel for a contour fit Quick-release buckle and zippered front entry for easy on and off Bellows front pocket with hook-and-loop closure provides plenty of storage for day-use essentials; Back shoulder lash point for attaching strobe light, fishing net, etc Hat loop also doubles as a hanging loop for drying your PFD Reflective padded shoulder straps provide added visibility and won't rub or chafe View all MTI Women's PFDsTypes InfographicFashion InfographicShoes DictionaryFashion Dictionary22 FashionShoes FashionFashion TipsMule 22Shoes 22ForwardCan you tell the difference between a slingback and a mule?

Now you can! | 22 Fashion Infographics You Need In Your Life Where is Planet Nine? There is an uneasy exhilaration in announcing that the solar system might contain a dim, massive, and as-yet unseen planet. Certainly, nearly every attempt to predict the existence of a “Planet X” has ended in failure, but history does contain one shining success. LeVerrier and Adams’ theoretical predictions of the existence of Neptune, based on observed irregularities in Uranus’ orbit, are hailed as one of the all-time success stories of astronomy. And as history shows, the issues with post-1846 claims of Planet X have had more to do with erroneous interpretation of the observational data, than anything else. In other words, every time the observations seemed to call for an introduction of a putative additional planet, further analysis has revealed that the apparent anomalies could be fully reconciled within the framework of the known solar system. Remarkably, the solar system in 2016 tells a very different story.

Beginning with the 2003 detection of Sedna (a discovery I remember learning about from a guy cautiously trying to hide his lit cigarette in his backpack during high school lunch break), it has been clear that the solar system still has some tricks up its sleeve. Unlike the rest of the Kuiper belt, Sedna traces out an orbit whose origin cannot be explained by perturbations from the known giant planets alone. And while Sedna’s isolated orbit could in principle be attributed to a dynamical perturbation that occurred during the solar system’s infancy, the 2014 paper by Trujillo and Sheppard demonstrated that there is in fact, much more to the story. It was with this very paper in hand, and a facial expression showing a combination of excitement and concern, that Mike Brown walked into my office a year and a half ago. Mike and I were genuinely perplexed. Could the confinement of the orbits be due to an observational bias or a mere coincidence (after all, we are talking about six objects here - not exactly “big data”)?

Thankfully, the probability of the observed alignment being fortuitous can be assessed in a statistically rigorous manner, and clocks in at right around 0.007%. Not a great gamble. Moreover, application of simple perturbation theory (or direct numerical integration) demonstrates that if allowed to evolve under the gravitational influence of Jupiter, Saturn, Uranus and Neptune, the orbits would become randomly oriented on timescales much shorter than than the multi-billion year lifetime of the solar system. So the dynamical origin of the peculiar structure of the Kuiper belt cannot be outsourced to the distant past - something is holding the orbits together right now. Our progress was initially anything but rapid. Coming from observational and theoretical backgrounds respectively, Mike and I don’t always speak the same language, and would spend hours arguing profusely, only to later realize that we are in fact, saying the exact same thing. Then there were all the ideas that did not pan out.

Ideas crowding out our outtakes reel range from models where the self-gravity of the Kuiper belt itself keeps the observed structure intact (see a recent paper by Madigan & McCourt on this topic) to a scenario where the orbit of a distant planet cradles the orbits of Kuiper belt objects from the outside, maintaining the same average orientation. Each hypothesis failed when confronted with the data. Last summer brought our first glimpse of hope. Through a series of numerical experiments (wherein an initially axisymmetric disk of planetesimals occupying eccentric, Neptune-hugging orbits, was allowed to evolve under the gravitational influence of a distant perturber) we began to note that planetesimal swarms could be sculpted into collinear groups of spatially confined orbits by “Planet Nine". Intriguingly, this would only occur if Planet Nine was chosen to be substantially more massive than the Earth, and to reside on a highly eccentric orbit. More unexpectedly, the confined orbits would cluster in a configuration where the long axes of their obits are anti-aligned with respect to Planet Nine, signaling that the dynamical mechanism at play is resonant in nature.