Expand Your World

We are citizens of a little world called University. It is the core of our lives; we live and breathe its rarified air. Its sidewalks carry us from one gray building to another- from applied art to zoology, with stopovers at child development and economics. Its professors cram our little heads with facts and figures- vapor pressure at sea level or the number of raisins in one cup

Add a Jibber To Your Wardrobe

Start now to knit a jibber to combat cold winter winds. A jibber is an easy-to-knit cap which protects head and ears, and yet is lightweight and uncumbersome. It is about five inches wide at the top of the head, narrows to two inches under the chin, and is fastened securely by yarn ties to keep out cold air

Conversation Carnations

With a few inexpensive materials and a little imagination, create table centerpieces which will be conversation pieces as well

Follow an Oriental Formula

There\u27s a simple formula to arranging flowers that has been handed down through the centuries by the Japanese. You can always be sure if you follow the rules

The Iowa Homemaker vol.39A, no.1

Follow an Oriental Formula, Marty Keeney, page 4 Planning + Imagination = Shower Success, Mary Jacobs Jensen, page 5 Gridiron Greats, Gail Devens, page 6 About Discount Houses, Carol Shellenbarger, page 7 Hem Yourself a Harem, Marcena Christian, page 8 Facial Focus, Marilyn Bratten, page 10 Does Your Equipment Measure Up?, Helen Rank, page 11 What’s Going On?, page 12 Inside Story, page 1

The Iowa Homemaker vol.39A, no.3

Halloween-Time for Fanciful Goodies, Rachel Davis, page 5 Checkerboard Summer, Jane Gibson, page 6 Imagination + Independence Encouraged By Honors Program, Carol Shellenbarger, page 8 Honoraries Stress Scholarship, Diane Houser, page 9 Have You Lost Your Marbles?, Carol Armstrong Wolf, page 10 Add a Jibber to Your Wardrobe, Marty Keeney, page 12 Dishpan Hands Soon Obsolete, Beth Beecher, page 13 Key to Personality – Your Walk, Suzanne Guernsey, page 14 How Do You Rate With Your Professor?, Mary Stoner, page 15 What’s Going On, page 1

The Iowa Homemaker vol.40, no.1

As Others See Us, Tom Emmerson, Beth Lambeth and Sue Guernsey, page 6 China Cues for Smart Shoppers, Doris Post, page 8 Reflections of You, Sylvia Noid, page 9 Campus Tours, Inc., Patty Anderson, page 10 Child Development Experts Study “Multiple Mother” Effects, Carol Calhoon, page 11 Behind the TV Camera, Carolynn DeLay, page 12 Gray Meals, One Subject of Food Technology, Mary Ellen Muckenhirn, page 14 Coed Chooses Spring Fashion’s Fancy, Laveda Jansonius, page 17 Expand Your World, Marty Keeney, page 18 RAIN, Diane Houser, page 21 What’s Going On?, Carol Shellenbarger, page 2

On the origin and evolution of the material in 67P/Churyumov-Gerasimenko

International audiencePrimitive objects like comets hold important information on the material that formed our solar system. Several comets have been visited by spacecraft and many more have been observed through Earth- and space-based telescopes. Still our understanding remains limited. Molecular abundances in comets have been shown to be similar to interstellar ices and thus indicate that common processes and conditions were involved in their formation. The samples returned by the Stardust mission to comet Wild 2 showed that the bulk refractory material was processed by high temperatures in the vicinity of the early sun. The recent Rosetta mission acquired a wealth of new data on the composition of comet 67P/Churyumov-Gerasimenko (hereafter 67P/C-G) and complemented earlier observations of other comets. The isotopic, elemental, and molecular abundances of the volatile, semi-volatile, and refractory phases brought many new insights into the origin and processing of the incorporated material. The emerging picture after Rosetta is that at least part of the volatile material was formed before the solar system and that cometary nuclei agglomerated over a wide range of heliocentric distances, different from where they are found today. Deviations from bulk solar system abundances indicate that the material was not fully homogenized at the location of comet formation, despite the radial mixing implied by the Stardust results. Post-formation evolution of the material might play an important role, which further complicates the picture. This paper discusses these major findings of the Rosetta mission with respect to the origin of the material and puts them in the context of what we know from other comets and solar system objects

Follow an Oriental Formula

There's a simple formula to arranging flowers that has been handed down through the centuries by the Japanese. You can always be sure if you follow the rules.</p