【香蕉面包】
by 毛毛妈
我们家领导们都喜欢香蕉，每次买一大把，来不及吃完都已经变熟了。用熟了的香蕉做香蕉面包，没有太多的技术含量，面包很湿润柔软，放了全麦面粉和燕麦，比较健康吧。
用料:
1：中筋面粉1杯（160克），全麦面粉1/2杯（80克），燕麦片1/2杯（47克）；
2：白糖1/4杯（52克），红糖1/4杯（45克）
3：泡打粉1又1/2茶匙（7克），小苏打1/3茶匙（1.5克），盐1/4茶匙，1又1/2茶匙肉桂粉；
4：核桃仁1/4杯（30克），压碎；
5：香蕉2根（净重204克）；
6：玉米油1/4杯（53克），杏仁奶或低脂白脱牛奶1/3杯（80克），香草香精1又1/4茶匙（6克）；
7：大鸡蛋2只。
其他：
9×5 英寸玻璃面包烤盘。
注：1大匙Tablespoon=15毫升，1茶匙Teaspoon=5毫升，1杯Cup=240毫升。
做法：
1、预热烤箱350F/175摄氏度。将所有1-4料放一盆里（图1），用一叉子拌匀（图2）待用。将香蕉放入另外一盆里，用勺子压碎，然后放入所有6-7料（图3），用打蛋器（handheld mixer）高速打2-3分钟（图4）到均匀（图5）。
2、将充分混合均匀的1-4料，倒入蛋糊里（图6），用打蛋器中速（图7）打30秒，还可以看到少许干粉（图8）。
3、然后用橡皮刀拌至刚刚均匀（图9），千万不要拌过头。玻璃面包烤盘喷上PAM不粘油，将面糊放入烤盘里（图10）。
4、将烤盘放入预热至350F/175摄氏度的烤箱内，烤50分钟左右至表面金黄色，用牙签插入，拿出是干净的就好了。
5、烤好的香蕉面包在烤盘里冷凉20分钟后，取出切块。可以热食，剩余的香蕉面包放一密闭盒里，室温下可以保存2-3天，冰箱可以冷藏1周。
The guide also invokes two different standard theories,
both of which have been discounted by art historians: that Mary Magdalene, somewhat than the apostle John, sits on Jesus’ right in Leonardo da Vinci’s “The Final Supper” painting, and that a disembodied hand in the painting holds a knife.
Brown’s story centers around the speculation that Jesus married his follower Mary
Magdalene, had a toddler with her, and that the descendants of that marriage reside in the present day.
Pesci’s theory and its attainable relationship to da Vinci’s mirror writing, whereas alluring, current some issues.
The newest principle du jour has generated so much pleasure that
a number of da Vinci-centered Web sites crashed from an overwhelming quantity of visitors.
Whatever required an excessive amount of gravity
and weight, we had to search out one other means to express that in swim,” explains Lignini. Doug. “They
were very complicated, because of all of the dreadlocks,
their tentacles. WOH 5170: One other luminary of the big Magellanic Cloud, WOH 5170 stands out for its
sheer dimension and is taken into account amongst the biggest stars found
on this satellite tv for pc galaxy of the Milky Approach.
Located in the large Magellanic Cloud, approximately
165,000 gentle years from Earth, R136a1 is a member of the rare class of hyper-massive
stars, weighing in at greater than 170 to 230 times the mass of our sun.
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